On the Dearth of Compact, Massive, Red Sequence Galaxies in the Local Universe (2009)
Taylor, Edward N, Franx, Marijn, Glazebrook, Karl, Brinchmann, Jarle, Van Der Wel, Arjen, Van Dokkum, Pieter G
Using data from the Sloan Digital Sky Survey (SDSS; data release 7), we have conducted a search for local analogs to the extremely compact, massive, quiescent galaxies that have been identified at z...
GRB 090426: The Environment of a Rest-Frame 0.35-second Gamma-Ray Burst at Redshift z=2.609 (2009)
Levesque, Emily M., Bloom, Joshua S., Butler, Nathaniel R., Perley, Daniel A., Cenko, S. Bradley, Prochaska, J. Xavier, ...
We present the discovery of an absorption-line redshift of z = 2.609 for GRB 090426, establishing the first firm lower limit to a redshift for a gamma-ray burst with an observed duration of 90%...
The WiggleZ Dark Energy Survey: small-scale clustering of Lyman-break galaxies at z < 1 (2009)
Blake, Chris, Jurek, Russell J., Brough, Sarah, Colless, Matthew, Couch, Warrick, Croom, Scott, ...
The WiggleZ Dark Energy Survey is a large-scale structure survey of intermediate-redshift ultraviolet-selected (UV-selected) emission-line galaxies scheduled to cover 1000 deg^2, spanning a broad...
A spectroscopic measure of the star-formation rate density in dwarf galaxies at z~1 (2009)
Davies, G. T., Gilbank, David, Glazebrook, Karl, Bower, Richard, Baldry, I. K., Balogh, Michael, ...
We use a K-selected (22.5 < K_AB < 24.0) sample of dwarf galaxies (8.4 < log(M*/Msun) < 10) at 0.89
Sumiyoshi, Masanao, Totani, Tomonori, Oshige, Shunsuke, Glazebrook, Karl, Akiyama, Masayuki, Morokuma, Tomoki, ...
Efficient selection of emission line galaxies at z > 1 by photometric information in wide field surveys is one of the keys for future spectroscopic surveys to constrain dark energy using the baryon...
The WiggleZ Dark Energy Survey: small-scale clustering of Lyman Break Galaxies at z < 1 (2009)
Blake, Chris, Jurek, Russell, Brough, Sarah, Colless, Matthew, Couch, Warrick, Croom, Scott, ...
The WiggleZ Dark Energy Survey is a large-scale structure survey of intermediate-redshift UV-selected emission-line galaxies scheduled to cover 1000 sq deg, spanning a broad redshift range 0.2 < z <...
Sumiyoshi, Masanao, Totani, Tomonori, Oshige, Shunsuke, Glazebrook, Karl, Akiyama, Masayuki, Morokuma, Tomoki, ...
Efficient selection of emission line galaxies at z > 1 by photometric information in wide field surveys is one of the keys for future spectroscopic surveys to constrain dark energy using the baryon...
Observations of the naked-eye GRB 080319B: implications of nature's brightest explosion (2009)
Bloom, J. S., Perley, D. A., Li, W., Butler, N. R., Miller, A. A., Kocevski, D., ...
The first gamma-ray burst (GRB) confirmed to be bright enough to be seen with the naked eye, GRB 080319B at redshift z = 0.937, allowed for exquisite follow-up observations across the electromagnetic...
The galaxy population hosting gamma-ray bursts (2009)
Savaglio, S., Glazebrook, Karl, Le Borgne, D.
We present the most extensive and complete study of the properties for the largest sample (46 objects) of gamma-ray burst (GRB) host galaxies. The redshift interval and the mean redshift of the...
Damjanov, Ivana, McCarthy, Patrick J., Abraham, Roberto G., Glazebrook, Karl, Yan, Haojing, Mentuch, Erin, ...
We present the results of Near-Infrared Camera and Multi-Object Spectrometer (NICMOS) imaging of a sample of 19 high-mass passively evolving galaxies with 1.2 < z < 2, taken primarily from the...
The WiggleZ Dark Energy Survey: small-scale clustering of Lyman-break galaxies at z < 1 (2009)
Blake, Chris, Jurek, Russell, Brough, Sarah, Colless, Matthew, Couch, Warrick, Croom, Scott M., ...
The WiggleZ Dark Energy Survey is a large-scale structure survey of intermediate-redshift ultraviolet-selected (UV-selected) emission-line galaxies scheduled to cover 1000 deg2, spanning a broad...
Mentuch, Erin, Abraham, Roberto G., Glazebrook, Karl, McCarthy, Patrick J., Yan, Haojing, O'Donnell, Daniel V., ...
A broad continuum excess in the near-infrared, peaking in the rest frame at 2-5 micron, is detected in a spectroscopic sample of 88 galaxies at 0.5
Red nuggets at z ~ 1.5: compact passive galaxies and the formation of the Kormendy relation (2009)
Damjanov, Ivana, McCarthy, Partick J., Abraham, Roberto G., Glazebrook, Karl, Yan, Haojing, Mentuch, Erin, ...
A spectroscopic measure of the star formation rate density in dwarf galaxies at z∼ 1 (2009)
Davies, G. T., Gilbank, David G., Glazebrook, Karl, Bower, Richard G., Baldry, I. K., Balogh, Michael L., ...
Sumiyoshi, Masanao, Totani, Tomonori, Oshige, Shunsuke, Glazebrook, Karl, Akiyama, Masayuki, Morokuma, Tomoki, ...
Efficient selection of emission line galaxies at z > 1 by photometric information in wide field surveys is one of the keys for future spectroscopic surveys to constrain dark energy using the baryon...
Observations of the naked-eye GRB 080319B: implications of nature's brightest explosion (2009)
Bloom, J. S., Perley, D. A., Li, W., Butler, N. R., Miller, A. A., Kocevski, D., ...
The first gamma-ray burst (GRB) confirmed to be bright enough to be seen with the naked eye, GRB 080319B at redshift z = 0.937, allowed for exquisite follow-up observations across the electromagnetic...
The galaxy population hosting gamma-ray bursts (2009)
Savaglio, S., Glazebrook, Karl, Le Borgne, D.
We present the most extensive and complete study of the properties for the largest sample (46 objects) of gamma-ray burst (GRB) host galaxies. The redshift interval and the mean redshift of the...
Damjanov, Ivana, McCarthy, Patrick J., Abraham, Roberto G., Glazebrook, Karl, Yan, Haojing, Mentuch, Erin, ...
We present the results of Near-Infrared Camera and Multi-Object Spectrometer (NICMOS) imaging of a sample of 19 high-mass passively evolving galaxies with 1.2 < z < 2, taken primarily from the Gemini...
The WiggleZ Dark Energy Survey: small-scale clustering of Lyman-break galaxies at z < 1 (2009)
Blake, Chris, Jurek, Russell, Brough, Sarah, Colless, Matthew, Couch, Warrick, Croom, Scott M., ...
The WiggleZ Dark Energy Survey is a large-scale structure survey of intermediate-redshift ultraviolet-selected (UV-selected) emission-line galaxies scheduled to cover 1000 deg2, spanning a broad...
Mentuch, Erin, Abraham, Roberto G., Glazebrook, Karl, McCarthy, Patrick J., Yan, Haojing, O'Donnell, Daniel V., ...
A broad continuum excess in the near-infrared, peaking in the rest frame at 2-5 micron, is detected in a spectroscopic sample of 88 galaxies at 0.5
Galaxy formation: too small to ignore (2009)
A study of one galaxy's dynamics backs up previous claims that surprisingly compact galaxies existed in the early Universe. But how such objects blew up in size to form present-day galaxies remains a...
The WiggleZ dark energy survey (2008)
Blake, Chris, Brough, Sarah, Couch, Warrick, Glazebrook, Karl, Poole, Greg, Davis, Tamara, ...
The accelerating expansion of the universe, attributed to "dark energy", has no accepted theoretical explanation. The origin of this phenomenon unambiguously implicates new physics via a novel form...
Mentuch, Erin, Scott, Alan, Abraham, Roberto, Barton, Elizabeth, Bershady, Matthew, Bland-Hawthorn, Joss, ...
The Flamingos-2 Tandem Tunable filter is a tunable, narrow-band filter, consisting of two Fabry-Perot etalons in series, capable of scanning to any wavelength from 0.95 to 1.35 microns with a...
Red Nuggets at z~1.5: Compact passive galaxies and the formation of the Kormendy Relation (2008)
Damjanov, Ivana, McCarthy, Patrick J., Abraham, Roberto G., Glazebrook, Karl, Yan, Haojing, Mentuch, Erin, ...
We present the results of NICMOS imaging of a sample of 16 high mass passively evolving galaxies with 1.32, this is the first time such systems have been detected in a rest-frame optical survey at 1.3
Galaxy Mass Growth in GDDS and SDSS (2008)
Glazebrook, Karl, Mentuch, Erin, McCarthy, Pat, Abraham, Roberto, Baldry, Ivan, Driver, Simon
I present some new results related to our understanding of the masses of galaxies both in the local and high-redshift Universe. At high-redshift new Spitzer data on galaxies in the Gemini Deep Deep...
The sixth data release of the Sloan Digital Sky Survey (2008)
Adelman-McCarthy, Jennifer K., Agüeros, Marcel A., Allam, Sahar S., Prieto, Carlos Allende, Anderson, Kurt S. J., Anderson, Scott F., ...
This paper describes the Sixth Data Release of the Sloan Digital Sky Survey. With this data release, the imaging of the northern Galactic cap is now complete. The survey contains images and...
Hoversten, E. A., Glazebrook, Karl
This paper revisits the classical Kennicutt method for inferring the stellar IMF from the integrated light properties of galaxies. The large-size, uniform high-quality data set from the SDSS DR4 is...
The sixth data release of the Sloan Digital Sky Survey (2008)
Adelman-McCarthy, Jennifer K., Agueros, Marcel A., Allam, Sahar S., Prieto, Carlos Alende, Anderson, Kurt S. J., Anderson, Scott F., ...
This paper describes the Sixth Data Release of the Sloan Digital Sky Survey. With this data release, the imaging of the northern Galactic cap is now complete. The survey contains images and...
Hoversten, E. A., Glazebrook, Karl
This paper revisits the classical Kennicutt method for inferring the stellar IMF from the integrated light properties of galaxies. The large-size, uniform high-quality data set from the SDSS DR4 is...
The sixth data release of the Sloan Digital Sky Survey (2008)
Adelman-McCarthy, Jennifer K., Agueros, Marcel A., Allam, Sahar S., Prieto, Carlos Alende, Anderson, Kurt S. J., Anderson, Scott F., ...
This paper describes the Sixth Data Release of the Sloan Digital Sky Survey. With this data release, the imaging of the northern Galactic cap is now complete. The survey contains images and...
The sixth data release of the sloan digital sky survey (2008)
Adelman-McCarthy, Jennifer K., Agüros, Marcel A., Allam, Sahar S., Allende Prieto, Carlos, Anderson, Kurt S. J., Anderson, Scott F., ...
Baldry, Ivan K., Glazebrook, Karl, Driver, Simon P.
A comparison between published field galaxy stellar mass functions (GSMFs) shows that the cosmic stellar mass density is in the range 4–8 per cent of the baryon density (assuming Ωb=...
Baldry, Ivan K., Glazebrook, Karl, Driver, Simon P.
A comparison between published field galaxy stellar mass functions (GSMFs) shows that the cosmic stellar mass density is in the range 4–8 per cent of the baryon density (assuming Ωb=...
Hoversten, E. A., Glazebrook, Karl
This paper revisits the classical Kennicutt method for inferring the stellar IMF from the integrated light properties of galaxies. The large-size, uniform high-quality data set from the SDSS DR4 is...
The sixth data release of the Sloan Digital Sky Survey (2008)
Adelman-McCarthy, Jennifer K., Agueros, Marcel A., Allam, Sahar S., Prieto, Carlos Alende, Anderson, Kurt S. J., Anderson, Scott F., ...
This paper describes the Sixth Data Release of the Sloan Digital Sky Survey. With this data release, the imaging of the northern Galactic cap is now complete. The survey contains images and...
Baldry, Ivan K., Glazebrook, Karl, Driver, Simon P.
A comparison between published field galaxy stellar mass functions (GSMFs) shows that the cosmic stellar mass density is in the range 4–8 per cent of the baryon density (assuming Ωb=...
Hoversten, E. A., Glazebrook, Karl
This paper revisits the classical Kennicutt method for inferring the stellar IMF from the integrated light properties of galaxies. The large-size, uniform high-quality data set from the SDSS DR4 is...
Baldry, Ivan K., Glazebrook, Karl, Driver, Simon P.
A comparison between published field galaxy stellar mass functions (GSMFs) shows that the cosmic stellar mass density is in the range 4–8 per cent of the baryon density (assuming Ωb=...
The WiggleZ dark energy survey (2008)
Blake, Chris, Brough, Sarah, Couch, Warrick J., Glazebrook, Karl, Poole, Greg, Davis, Tamara M., ...
The accelerating expansion of the universe, attributed to 'dark energy', has no accepted theoretical explanation. The origin of this phenomenon unambiguously implicates new physics via a novel form...
Four faint T dwarfs from the UKIRT Infrared Deep Sky Surveys (UKIDSS) Southern Stripe (2008)
Chiu, Kuenley, Liu, Michael C., Jiang, Linhua, Allers, Katelyn N., Stark, Daniel P., Bunker, Andrew, ...
We present the optical and near-infrared photometry and spectroscopy of four faint T dwarfs newly discovered from the UKIDSS first data release. The sample, drawn from an imaged area of ∼136...
From HI to HII: enabling deep and wide optical redshift surveys matched to ASKAP (2008)
Abstract not available.
The WiggleZ dark energy survey (2008)
Blake, Chris, Brough, Sarah, Couch, Warrick, Glazebrook, Karl, Poole, Greg, Davis, Tamara, ...
The accelerating expansion of the universe, attributed to "dark energy", has no accepted theoretical explanation. The origin of this phenomenon unambiguously implicates new physics via a novel form...
Mentuch, Erin, Scott, Alan D., Abraham, Roberto G., Barton, Elizabeth J., Bershady, Matthew A., Bland-Hawthorn, Joss, ...
Abstract not available.
The sixth data release of the Sloan Digital Sky Survey (2008)
Adelman-McCarthy, Jennifer K., Agueros, Marcel A., Allam, Sahar S., Prieto, Carlos Alende, Anderson, Kurt S. J., Anderson, Scott F., ...
This paper describes the Sixth Data Release of the Sloan Digital Sky Survey. With this data release, the imaging of the northern Galactic cap is now complete. The survey contains images and...
Hoversten, E. A., Glazebrook, Karl
This paper revisits the classical Kennicutt method for inferring the stellar IMF from the integrated light properties of galaxies. The large-size, uniform high-quality data set from the SDSS DR4 is...
Baldry, Ivan K., Glazebrook, Karl, Driver, Simon P.
A comparison between published field galaxy stellar mass functions (GSMFs) shows that the cosmic stellar mass density is in the range 4–8 per cent of the baryon density (assuming Ωb=...
The WiggleZ dark energy survey (2008)
Blake, Chris, Brough, Sarah, Couch, Warrick J., Glazebrook, Karl, Poole, Gregory B., Davis, Tamara M., ...
The accelerating expansion of the universe, attributed to 'dark energy', has no accepted theoretical explanation. The origin of this phenomenon unambiguously implicates new physics via a novel form...
Four faint T dwarfs from the UKIRT Infrared Deep Sky Surveys (UKIDSS) Southern Stripe (2008)
Chiu, Kuenley, Liu, Michael C., Jiang, Linhua, Allers, Katelyn N., Stark, Daniel P., Bunker, Andrew, ...
We present the optical and near-infrared photometry and spectroscopy of four faint T dwarfs newly discovered from the UKIDSS first data release. The sample, drawn from an imaged area of ∼136 deg2...
From HI to HII: enabling deep and wide optical redshift surveys matched to ASKAP (2008)
Abstract not available.
Mentuch, Erin, Scott, Alan D., Abraham, Roberto G., Barton, Elizabeth J., Bershady, Matthew A., Bland-Hawthorn, Joss, ...
Abstract not reproduced here by request of the publisher. The text is available from: http://dx.doi.org/10.1117/12.789692.
Four Faint T Dwarfs from the UKIRT Infrared Deep Sky Survey (UKIDSS) Southern Stripe (2007)
Chiu, Kuenley, Liu, Michael C., Jiang, Linhua, Allers, Katelyn N., Stark, Daniel P., Bunker, Andrew, ...
We present the optical and near-infrared photometry and spectroscopy of four faint T dwarfs newly discovered from the UKIDSS first data release. The sample, drawn from an imaged area of ~136 square...
as an Astronomer-Friendly Language---the (2007)
Pgperl Experience, George H. Jacoby, Jeannette Barnes, Karl Glazebrook
. Interest has focused in the last year on the use of high level `glue' languages from outside the community for astronomical applications. The canonical example is the popular TCL language...
Accepted for publication in Monthly Notices of the R.A.S. (2007)
Karl Glazebrook, J. A. Peacock, L. Miller, C. A. Collins
An imaging K-band survey-- II: The redshift survey and galaxy evolution in the infrared
Hoversten, Erik A., Glazebrook, Karl
This paper revisits the classical Kennicutt method for inferring the stellar initial mass function (IMF) from the integrated light properties of galaxies. The large size, uniform high quality data...
A compact cluster of massive red galaxies at a redshift of 1.5 (2007)
McCarthy, Patrick J., Yan, Haojing, Abraham, Roberto G., Mentuch, Erin, Glazebrook, Karl, Yan, Lin, ...
We describe a compact cluster or group of massive red galaxies at z = 1.5 discovered in one of the Gemini Deep Deep Survey (GDDS) fields. Deep H-band imaging from the Hubble Space Telescope (HST)...
Optimising Baryon Acoustic Oscillation Surveys - I: Testing the concordance LCDM cosmology (2007)
Parkinson, David, Blake, Chris, Kunz, Martin, Bassett, Bruce A., Nichol, Robert C., Glazebrook, Karl
We optimize the design of future spectroscopic redshift surveys for constraining the dark energy via precision measurements of the baryon acoustic oscillations (BAO), with particular emphasis on the...
The WiggleZ project: AAOmega and Dark Energy (2007)
Glazebrook, Karl, Blake, Chris, Couch, Warrick, Forbes, Duncan, Drinkwater, Michael, Jurek, Russell, ...
We describe the `WiggleZ' spectroscopic survey of 280,000 star-forming galaxies selected from a combination of GALEX ultra-violet and SDSS + RCS2 optical imaging. The fundamental goal is a detection...
The Gemini Deep Deep Survey: VIII. When Did Early-type Galaxies Form? (2007)
Abraham, Roberto G., Nair, Preethi, McCarthy, Patrick J., Glazebrook, Karl, Mentuch, Erin, Yan, Haojing, ...
We have used the Hubble Space Telescope's Advanced Camera for Surveys (Ford et al. 2003) to measure the cumulative mass density in morphologically-selected early-type galaxies over the redshift range...
The GLARE Survey II. Faint z=6 Ly-alpha Line Emitters in the HUDF (2007)
Stanway, Elizabeth R, Bunker, Andrew J, Glazebrook, Karl, Abraham, Roberto G, Rhoads, James, Malhotra, Sangeeta, ...
The galaxy population at z~6 has been the subject of intense study in recent years, culminating in the Hubble Ultra Deep Field (HUDF) -- the deepest imaging survey yet. A large number of high...
When do early-type galaxies form? (2007)
Abraham, Roberto G., McCarthy, Patrick J., Mentuch, Erin, Glazebrook, Karl, Nair, Preethi, Gauthier, Jean-René, ...
GHostS - Gamma-ray burst Host Studies (2007)
Savaglio, Sandra, Budavári, Tamás, Glazebrook, Karl, Le Borgne, Damien, Le Floc'h, Emeric, Chen, Hsiao-Wen, ...
A compact cluster of massive red galaxies at a redshift of 1.5 (2007)
McCarthy, Patrick J., Yan, Haojing, Abraham, Roberto G., Mentuch, Erin, Glazebrook, Karl, Yan, Lin, ...
Optimizing baryon acoustic oscillation surveys I : testing the concordance (2007)
Parkinson, David R., Blake, Christopher A., Kunz, Martin, Bassett, Bruce A., Nichol, Robert C., Glazebrook, Karl, ...
We optimize the design of future spectroscopic redshift surveys for constraining the dark energy via precision measurements of the baryon acoustic oscillations (BAOs), with particular emphasis on the...
The fifth data release of the sloan digital sky survey (2007)
Adelman-McCarthy, Jennifer K., Agüeros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., Annis, James, ...
The Gemini deep deep survey - VIII. When did early‐type galaxies form? (2007)
Abraham, Roberto G., Nair, Preethi, McCarthy, Patrick J., Glazebrook, Karl, Mentuch, Erin, Yan, Haojing, ...
The Fifth Data Release of the Sloan Digital Sky Survey (2007)
Adelman-McCarthy, Jennifer K., Agüeros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., Annis, James, ...
This paper describes the Fifth Data Release (DR5) of the Sloan Digital Sky Survey (SDSS). DR5 includes all survey quality data taken through 2005 June and represents the completion of the SDSS-I...
Optimizing baryon acoustic oscillation surveys I: testing the concordance (2007)
Parkinson, David, Blake, Chris, Kunz, Martin, Bassett, Bruce A., Nichol, Robert C., Glazebrook, Karl
We optimize the design of future spectroscopic redshift surveys for constraining the dark energy via precision measurements of the baryon acoustic oscillations (BAOs), with particular emphasis on the...
The Gemini Deep Deep Survey VIII : when did early-type galaxies form? (2007)
Abraham, Roberto G., Nair, Preethi, McCarthy, Patrick J., Glazebrook, Karl, Mentuch, Erin, Yan, Haojing, ...
We have used the Hubble Space Telescope's Advanced Camera for Surveys (Ford et al. 2003) to measure the cumulative mass density in morphologically selected early-type galaxies over the redshift range...
The fifth data release of the Sloan Digital Sky Survey (2007)
Adelman-McCarthy, Jennifer K., Agueros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., Annis, James, ...
This paper describes the Fifth Data Release (DR5) of the Sloan Digital Sky Survey (SDSS). DR5 includes all survey quality data taken through 2005 June and represents the completion of the SDSS-I...
A compact cluster of massive red galaxies at a redshift of 1.5 (2007)
McCarthy, Patrick J., Yan, Haojing, Abraham, Roberto G., Mentuch, Erin, Glazebrook, Karl, Yan, Lin, ...
We describe a compact cluster or group of massive red galaxies at z = 1.5 discovered in one of the Gemini Deep Deep Survey (GDDS) fields. Deep H-band imaging from the Hubble Space Telescope (HST)...
Parkinson, David, Blake, Chris, Kunz, Martin, Bassett, Bruce A., Nichol, Robert C., Glazebrook, Karl
We optimize the design of future spectroscopic redshift surveys for constraining the dark energy via precision measurements of the baryon acoustic oscillations (BAOs), with particular emphasis on the...
The GLARE Survey II : faint z approximate to 6 Ly alpha line emitters in the HUDF (2007)
Stanway, Elizabeth R., Bunker, Andrew J., Glazebrook, Karl, Abraham, Roberto G., Rhoads, James, Malhotra, Sangeeta, ...
The galaxy population at z approximate to 6 has been the subject of intense study in recent years, culminating in the Hubble Ultra Deep Field (HUDF) - the deepest imaging survey yet. A large number...
Optimizing baryon acoustic oscillation surveys I : testing the concordance (2007)
Parkinson, David R., Blake, Christopher A., Kunz, Martin, Bassett, Bruce A., Nichol, Robert C., Glazebrook, Karl
We optimize the design of future spectroscopic redshift surveys for constraining the dark energy via precision measurements of the baryon acoustic oscillations (BAOs), with particular emphasis on the...
The Gemini Deep Deep Survey VIII : when did early-type galaxies form? (2007)
Abraham, Roberto G., Nair, Preethi, McCarthy, Patrick J., Glazebrook, Karl, Mentuch, Erin, Yan, Haojing, ...
We have used the Hubble Space Telescope's Advanced Camera for Surveys (Ford et al. 2003) to measure the cumulative mass density in morphologically selected early-type galaxies over the redshift range...
The Fifth Data Release of the Sloan Digital Sky Survey (2007)
Adelman-McCarthy, Jennifer K., Agueeros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., Annis, James, ...
This paper describes the Fifth Data Release (DR5) of the Sloan Digital Sky Survey (SDSS). DR5 includes all survey quality data taken through 2005 June and represents the completion of the SDSS-I...
A compact cluster of massive red galaxies at a redshift of 1.5 (2007)
McCarthy, Patrick J., Yan, Haojing, Abraham, Roberto G., Mentuch, Erin, Glazebrook, Karl, Yan, Lin, ...
We describe a compact cluster or group of massive red galaxies at z = 1.5 discovered in one of the Gemini Deep Deep Survey (GDDS) fields. Deep H-band imaging from the Hubble Space Telescope (HST)...
Parkinson, David, Blake, Chris, Kunz, Martin, Bassett, Bruce A., Nichol, Robert C., Glazebrook, Karl
We optimize the design of future spectroscopic redshift surveys for constraining the dark energy via precision measurements of the baryon acoustic oscillations (BAOs), with particular emphasis on the...
The GLARE Survey II : faint z approximate to 6 Ly alpha line emitters in the HUDF (2007)
Stanway, Elizabeth R., Bunker, Andrew J., Glazebrook, Karl, Abraham, Roberto G., Rhoads, James, Malhotra, Sangeeta, ...
The galaxy population at z approximate to 6 has been the subject of intense study in recent years, culminating in the Hubble Ultra Deep Field (HUDF) - the deepest imaging survey yet. A large number...
The WiggleZ Project: AAOmega and dark energy (2007)
Glazebrook, Karl, Blake, Christopher A., Couch, Warrick J., Forbes, Duncan A., Drinkwater, Michael J., Jurek, Russell, ...
We describe the 'WiggleZ' spectroscopic survey of 400,000 star-forming galaxies selected from a combination of GALEX ultra-violet and SDSS + RCS2 optical imaging. The fundamental goal is a detection...
Optimizing baryon acoustic oscillation surveys I : testing the concordance (2007)
Parkinson, David R., Blake, Christopher A., Kunz, Martin, Bassett, Bruce A., Nichol, Robert C., Glazebrook, Karl
We optimize the design of future spectroscopic redshift surveys for constraining the dark energy via precision measurements of the baryon acoustic oscillations (BAOs), with particular emphasis on the...
The Gemini Deep Deep Survey VIII : when did early-type galaxies form? (2007)
Abraham, Roberto G., Nair, Preethi, McCarthy, Patrick J., Glazebrook, Karl, Mentuch, Erin, Yan, Haojing, ...
We have used the Hubble Space Telescope's Advanced Camera for Surveys (Ford et al. 2003) to measure the cumulative mass density in morphologically selected early-type galaxies over the redshift range...
The Fifth Data Release of the Sloan Digital Sky Survey (2007)
Adelman-McCarthy, Jennifer K., Agueeros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., Annis, James, ...
This paper describes the Fifth Data Release (DR5) of the Sloan Digital Sky Survey (SDSS). DR5 includes all survey quality data taken through 2005 June and represents the completion of the SDSS-I...
Parkinson, David, Blake, Chris, Kunz, Martin, Bassett, Bruce A., Nichol, Robert C., Glazebrook, Karl
We optimize the design of future spectroscopic redshift surveys for constraining the dark energy via precision measurements of the baryon acoustic oscillations (BAOs), with particular emphasis on the...
The GLARE Survey II : faint z approximate to 6 Ly alpha line emitters in the HUDF (2007)
Stanway, Elizabeth R., Bunker, Andrew J., Glazebrook, Karl, Abraham, Roberto G., Rhoads, James, Malhotra, Sangeeta, ...
The galaxy population at z approximate to 6 has been the subject of intense study in recent years, culminating in the Hubble Ultra Deep Field (HUDF) - the deepest imaging survey yet. A large number...
A compact cluster of massive red galaxies at a redshift of 1.5 (2007)
McCarthy, Patrick J., Yan, Haojing, Abraham, Roberto G., Mentuch, Erin, Glazebrook, Karl, Yan, Lin, ...
We describe a compact cluster or group of massive red galaxies at z = 1.5 discovered in one of the Gemini Deep Deep Survey (GDDS) fields. Deep H-band imaging from the Hubble Space Telescope (HST)...
The WiggleZ Project: AAOmega and dark energy (2007)
Glazebrook, Karl, Blake, Christopher A., Couch, Warrick J., Forbes, Duncan A., Drinkwater, Michael J., Jurek, Russell, ...
We describe the 'WiggleZ' spectroscopic survey of 400,000 star-forming galaxies selected from a combination of GALEX ultra-violet and SDSS + RCS2 optical imaging. The fundamental goal is a detection...
The WiggleZ Project: AAOmega and dark energy (2007)
Glazebrook, Karl, Blake, Chris, Couch, Warrick J., Forbes, Duncan A., Drinkwater, Michael J., Jurek, Russell, ...
We describe the 'WiggleZ' spectroscopic survey of 400,000 star-forming galaxies selected from a combination of GALEX ultra-violet and SDSS + RCS2 optical imaging. The fundamental goal is a detection...
Parkinson, David, Blake, Chris, Kunz, Martin, Bassett, Bruce A., Nichol, Robert C., Glazebrook, Karl
We optimize the design of future spectroscopic redshift surveys for constraining the dark energy via precision measurements of the baryon acoustic oscillations (BAOs), with particular emphasis on the...
The GLARE Survey II : faint z approximate to 6 Ly alpha line emitters in the HUDF (2007)
Stanway, Elizabeth R., Bunker, Andrew J., Glazebrook, Karl, Abraham, Roberto G., Rhoads, James, Malhotra, Sangeeta, ...
The galaxy population at z approximate to 6 has been the subject of intense study in recent years, culminating in the Hubble Ultra Deep Field (HUDF) - the deepest imaging survey yet. A large number...
When do early-type galaxies form? (2007)
Abraham, Roberto G., McCarthy, Patrick J., Mentuch, Erin, Glazebrook, Karl, Nair, Preethi, Gauthier, Jean-Ren, ...
We have used the Hubble Space Telescope's Advanced Camera for Surveys to measure the mass density function of morphologically-selected early-type galaxies in the Gemini Deep Deep Survey fields, over...
The WiggleZ Project: AAOmega and dark energy (2007)
Glazebrook, Karl, Blake, Chris, Couch, Warrick J., Forbes, Duncan A., Drinkwater, Michael J., Jurek, Russell, ...
We describe the 'WiggleZ' spectroscopic survey of 400,000 star-forming galaxies selected from a combination of GALEX ultra-violet and SDSS + RCS2 optical imaging. The fundamental goal is a detection...
A compact cluster of massive red galaxies at a redshift of 1.5 (2007)
McCarthy, Patrick J., Yan, Haojing, Abraham, Roberto G., Mentuch, Erin, Glazebrook, Karl, Yan, Lin, ...
We describe a compact cluster or group of massive red galaxies at z = 1.5 discovered in one of the Gemini Deep Deep Survey (GDDS) fields. Deep H-band imaging from the Hubble Space Telescope (HST)...
Parkinson, David, Blake, Chris, Kunz, Martin, Bassett, Bruce A., Nichol, Robert C., Glazebrook, Karl
We optimize the design of future spectroscopic redshift surveys for constraining the dark energy via precision measurements of the baryon acoustic oscillations (BAOs), with particular emphasis on the...
The GLARE Survey II : faint z approximate to 6 Ly alpha line emitters in the HUDF (2007)
Stanway, Elizabeth R., Bunker, Andrew J., Glazebrook, Karl, Abraham, Roberto G., Rhoads, James, Malhotra, Sangeeta, ...
The galaxy population at z approximate to 6 has been the subject of intense study in recent years, culminating in the Hubble Ultra Deep Field (HUDF) - the deepest imaging survey yet. A large number...
The Gemini Deep Deep Survey VIII : when did early-type galaxies form? (2007)
Abraham, Roberto G., Nair, Preethi, McCarthy, Patrick J., Glazebrook, Karl, Mentuch, Erin, Yan, Haojing, ...
We have used the Hubble Space Telescope's Advanced Camera for Surveys (Ford et al. 2003) to measure the cumulative mass density in morphologically selected early-type galaxies over the redshift range...
The fifth data release of the Sloan Digital Sky Survey (2007)
Adelman-McCarthy, Jennifer K., Agueros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., Annis, James, ...
This paper describes the Fifth Data Release (DR5) of the Sloan Digital Sky Survey (SDSS). DR5 includes all survey quality data taken through 2005 June and represents the completion of the SDSS-I...
When do early-type galaxies form? (2007)
Abraham, Roberto G., McCarthy, Patrick J., Mentuch, Erin, Glazebrook, Karl, Nair, Preethi, Gauthier, Jean-Ren, ...
We have used the Hubble Space Telescope's Advanced Camera for Surveys to measure the mass density function of morphologically-selected early-type galaxies in the Gemini Deep Deep Survey fields, over...
Brown dwarfs and high-redshift quasars in the UKIDSS? Unlikely neighbors in the infrared (2007)
Chiu, Kuenley, Bunker, Andrew J., Glazebrook, Karl, Jiang, Linhua, Fan, Xiaohui, Fan, Xiaohui, ...
Over the ~ 5 years of its full operations, the SDSS rapidly broke high redshift quasar and brown dwarf discovery barriers by exploiting the advantages of the near-infrared/optical z filter, combined...
Cosmological constraints from the SDSS luminous red galaxies (2006)
Tegmark, Max, Eisenstein, Daniel J., Strauss, Michael A., Weinberg, David H., Blanton, Michael R., Frieman, Joshua A., ...
We measure the large-scale real-space power spectrum P(k) using luminous red galaxies (LRGs) in the Sloan Digital Sky Survey (SDSS) and use this measurement to sharpen constraints on cosmological...
Cosmological constraints from the SDSS Luminous Red Galaxies (2006)
Tegmark, Max, Eisenstein, Daniel, Strauss, Michael, Weinberg, David, Blanton, Michael, Frieman, Joshua, ...
Also archived in: arXiv:astro-ph/0608632 v2 Oct 30 2006
When do early-type galaxies form? (2006)
Abraham, Roberto G., McCarthy, Patrick J., Mentuch, Erin, Glazebrook, Karl, Nair, Preethi, Gauthier, Jean-Rene, ...
We have used the Hubble Space Telescope's Advanced Camera for Surveys to measure the mass density function of morphologically selected early-type galaxies in the Gemini Deep Deep Survey fields, over...
AAT Imaging and Microslit Spectroscopy in the Southern Hubble Deep Field (2006)
Glazebrook, Karl, Verma, Aprajita, Boyle, Brian, Oliver, Sebastian, Mann, Robert G., Monbleau, Davienne
We present a deep photometric (B- and R-band) catalog and an associated spectroscopic redshift survey conducted in the vicinity of the Hubble Deep Field South. The spectroscopy yields 53...
The fourth data release of the sloan digital sky survey (2006)
Adelman-McCarthy, Jennifer K., Agüeros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., Annis, James, ...
The fourth data release of the sloan digital sky survey (2006)
Adelman-McCarthy, Jennifer K., Agüeros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., Annis, James, ...
The fourth data release of the sloan digital sky survey (2006)
Adelman-McCarthy, Jennifer K., Agüeros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., Annis, James, ...
Glazebrook, Karl, Verma, Aprajita, Boyle, Brian, Oliver, Sebastian, Mann, Robert G., Monbleau, Davienne
The Fourth Data Release of the Sloan Digital Sky Survey (2006)
Adelman-McCarthy, Jennifer K., Agüeros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., Annis, James, ...
This paper describes the Fourth Data Release of the Sloan Digital Sky Survey (SDSS), including all survey-quality data taken through 2004 June. The data release includes five-band photometric data...
The WiggleZ Dark Energy Survey: 1000 redshifts and beyond (2006)
Drinkwater, Michael J., Pimbblet, Kevin, Jurek, Russell, Blake, Christopher A., Glazebrook, Karl, Woods, David, ...
Here we outline design aspects and first results of the WiggleZ Dark Energy Survey that has recently been awarded long-term status on the AAT from the 2006B semester. The primary aim of the WiggleZ...
The WiggleZ Dark Energy Survey: 1000 redshifts and beyond (2006)
Drinkwater, Michael J., Pimbblet, Kevin, Jurek, Russell, Blake, Christopher A., Glazebrook, Karl, Woods, David, ...
Here we outline design aspects and first results of the WiggleZ Dark Energy Survey that has recently been awarded long-term status on the AAT from the 2006B semester. The primary aim of the WiggleZ...
The WiggleZ Dark Energy Survey: 1000 redshifts and beyond (2006)
Drinkwater, Michael J., Pimbblet, Kevin, Jurek, Russell, Blake, Chris, Glazebrook, Karl, Woods, David, ...
Here we outline design aspects and first results of the WiggleZ Dark Energy Survey that has recently been awarded long-term status on the AAT from the 2006B semester. The primary aim of the WiggleZ...
Galaxy bimodality versus stellar mass and environment (2006)
Baldry, Ivan K., Balogh, Michael L., Bower, Richard G., Glazebrook, Karl, Nichol, Robert C., Bamford, S. P., ...
Abstract not available.
Gemini Deep Deep Survey. VI: massive Hδ-strong Galaxies at z 1 (2006)
Le Borgne, Damien, Abraham, Roberto G., Daniel, Kathryne J., McCarthy, Patrick J., Glazebrook, Karl, Savaglio, Sandra, ...
Abstract not available.
The fourth data release of the Sloan Digital Sky Survey (2006)
Adelman-McCarthy, Jennifer K., Agueros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., Annis, James, ...
This paper describes the Fourth Data Release of the Sloan Digital Sky Survey (SDSS), including all survey-quality data taken through 2004 June. The data release includes five-band photometric data...
Galaxy bimodality versus stellar mass and environment (2006)
Baldry, Ivan K., Balogh, Michael L., Bower, Richard G., Glazebrook, Karl, Nichol, Robert C., Bamford, S. P., ...
Abstract not available.
Gemini Deep Deep Survey. VI: massive Hδ-strong Galaxies at z 1 (2006)
Le Borgne, Damien, Abraham, Roberto G, Daniel, Kathryne J., McCarthy, Patrick J, Glazebrook, Karl, Savaglio, Sandra, ...
Abstract not available.
The fourth data release of the Sloan Digital Sky Survey (2006)
Adelman-McCarthy, Jennifer K., Agueros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., Annis, James, ...
This paper describes the Fourth Data Release of the Sloan Digital Sky Survey (SDSS), including all survey-quality data taken through 2004 June. The data release includes five-band photometric data...
Universal fitting formulae for baryon oscillation surveys (2006)
Blake, Chris, Parkinson, David, Bassett, Bruce A., Glazebrook, Karl, Kunz, Martin, Nichol, Robert C.
The next generation of galaxy surveys will attempt to measure the baryon oscillations in the clustering power spectrum with high accuracy. These oscillations encode a preferred scale which may be...
Glazebrook, Karl, Verma, Aprajita, Boyle, Brian J., Oliver, S., Mann, Robert G., Monbleau, Davienne
We present a deep photometric (B- and R-band) catalog and an associated spectroscopic redshift survey conducted in the vicinity of the Hubble Deep Field-South. The spectroscopy yields 53...
Cosmological constraints from the SDSS luminous red galaxies (2006)
Tegmark, Max, Eisenstein, Daniel J., Strauss, Michael A., Weinberg, David H., Blanton, Michael R., Frieman, Joshua A., ...
We measure the large-scale real-space power spectrum P(k) using luminous red galaxies (LRGs) in the Sloan Digital Sky Survey (SDSS) and use this measurement to sharpen constraints on cosmological...
Universal fitting formulae for baryon oscillation surveys (2006)
Blake, Christopher A., Parkinson, David R., Bassett, Bruce A., Glazebrook, Karl, Kunz, Martin, Nichol, Robert C.
The next generation of galaxy surveys will attempt to measure the baryon oscillations in the clustering power spectrum with high accuracy. These oscillations encode a preferred scale which may be...
Glazebrook, Karl, Verma, Aprajita, Boyle, Brian J., Oliver, S., Mann, Robert G., Monbleau, Davienne
We present a deep photometric (B- and R-band) catalog and an associated spectroscopic redshift survey conducted in the vicinity of the Hubble Deep Field-South. The spectroscopy yields 53...
Cosmological constraints from the SDSS luminous red galaxies (2006)
Tegmark, Max, Eisenstein, Daniel J., Strauss, Michael A., Weinberg, David H., Blanton, Michael R., Frieman, Joshua A., ...
We measure the large-scale real-space power spectrum P(k) using luminous red galaxies (LRGs) in the Sloan Digital Sky Survey (SDSS) and use this measurement to sharpen constraints on cosmological...
Design of a multi-object, high throughput, low resolution fiber spectrograph for WFMOS (2006)
Smee, Stephen A., Barkhouser, Robert H., Glazebrook, Karl
Abstract not reproduced here by request of the publisher. The text is available from: http://dx.doi.org/10.1117/12.672186.
The WiggleZ Dark Energy Survey: 1000 redshifts and beyond (2006)
Drinkwater, Michael J., Pimbblet, Kevin, Jurek, Russell, Blake, Chris, Glazebrook, Karl, Woods, David, ...
Here we outline design aspects and first results of the WiggleZ Dark Energy Survey that has recently been awarded long-term status on the AAT from the 2006B semester. The primary aim of the WiggleZ...
Galaxy bimodality versus stellar mass and environment (2006)
Baldry, Ivan K., Balogh, Michael L., Bower, Richard G., Glazebrook, Karl, Nichol, Robert C., Bamford, S. P., ...
Abstract not available.
Gemini Deep Deep Survey. VI: massive Hδ-strong Galaxies at z 1 (2006)
Le Borgne, Damien, Abraham, Roberto G., Daniel, Kathryne J., McCarthy, Patrick J., Glazebrook, Karl, Savaglio, Sandra, ...
Abstract not available.
The fourth data release of the Sloan Digital Sky Survey (2006)
Adelman-McCarthy, Jennifer K., Agueros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., Annis, James, ...
This paper describes the Fourth Data Release of the Sloan Digital Sky Survey (SDSS), including all survey-quality data taken through 2004 June. The data release includes five-band photometric data...
Universal fitting formulae for baryon oscillation surveys (2006)
Blake, Chris, Parkinson, David, Bassett, Bruce A., Glazebrook, Karl, Kunz, Martin, Nichol, Robert C.
The next generation of galaxy surveys will attempt to measure the baryon oscillations in the clustering power spectrum with high accuracy. These oscillations encode a preferred scale which may be...
Glazebrook, Karl, Verma, Aprajita, Boyle, Brian J., Oliver, S., Mann, Robert G., Monbleau, Davienne
We present a deep photometric (B- and R-band) catalog and an associated spectroscopic redshift survey conducted in the vicinity of the Hubble Deep Field-South. The spectroscopy yields 53...
Cosmological constraints from the SDSS luminous red galaxies (2006)
Tegmark, Max, Eisenstein, Daniel J., Strauss, Michael A., Weinberg, David H., Blanton, Michael R., Frieman, Joshua A., ...
We measure the large-scale real-space power spectrum P(k) using luminous red galaxies (LRGs) in the Sloan Digital Sky Survey (SDSS) and use this measurement to sharpen constraints on cosmological...
Design of a multi-object, high throughput, low resolution fiber spectrograph for WFMOS (2006)
Smee, Stephen A., Barkhouser, Robert H., Glazebrook, Karl
Abstract not reproduced here by request of the publisher. The text is available from: http://dx.doi.org/10.1117/12.672186.
Eisenstein, Daniel, Zehavi, Idit, Hogg, David, Scoccimarro, Roman, Blanton, Michael, Nichol, Robert, ...
Also archived in: arXiv:astro-ph/0501171 v1 10 Jan 2005
Universal fitting formulae for baryon oscillation surveys (2005)
Blake, Chris, Parkinson, David, Bassett, Bruce, Glazebrook, Karl, Kunz, Martin, Nichol, Robert C.
The next generation of galaxy surveys will attempt to measure the baryon oscillations in the clustering power spectrum with high accuracy. These oscillations encode a preferred scale which may be...
Hilton, Matt, Collins, Chris, De Propris, Roberto, Baldry, Ivan K., Baugh, Carlton M., Bland-Hawthorn, Joss, ...
The ROSAT-ESO Flux Limited X-ray (REFLEX) galaxy cluster survey and the 2dF Galaxy Redshift Survey (2dFGRS) respectively comprise the largest, homogeneous X-ray selected cluster catalogue and...
Glazebrook, Karl, Eisenstein, Daniel, Dey, Arjun, Nichol, Bob
This white paper gives an overview of the proposed Gemini/Subaru Wide-Field Multi-Object Spectrograph (WFMOS) and the proposed redshift surveys of 2.6 million galaxies with 0.5
Glazebrook, Karl, Blake, Chris
We use Monte Carlo techniques to simulate the ability of future large high-redshift galaxy surveys to measure the temporal evolution of the dark energy equation-of-state w(z), using the baryonic...
The Color Selection of Quasars from Redshifts 5 to 10: Cloning and Discovery (2005)
Chiu, Kuenley, Zheng, Wei, Schneider, Donald P., Glazebrook, Karl, Iye, Masanori, Kashikawa, Nobunari, ...
We present simulations of quasar colors, magnitudes, and numbers at redshifts 54.7 quasars increases by a factor of 3X by extending 0.7 i-magnitudes deeper than the SDSS spectroscopic survey limit of...
Gemini Deep Deep Survey VI: Massive Hdelta-strong galaxies at z=1 (2005)
Borgne, Damien Le, Abraham, Roberto, Daniel, Kathryne, McCarthy, Patrick, Glazebrook, Karl, Savaglio, Sandra, ...
We show that there has been a dramatic decline in the abundance of massive galaxies with strong Hdelta stellar absorption lines from z=1.2 to the present. These ``Hdelta-strong'', or HDS, galaxies...
The third data release of the sloan digital sky survey (2005)
Abazajian, Kevork, Adelman-McCarthy, Jennifer K., Agüeros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., ...
The Third Data Release of the Sloan Digital Sky Survey (2005)
Abazajian, Kevork, Adelman-McCarthy, Jennifer K., Agüeros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., ...
The Third Data Release of the Sloan Digital Sky Survey (2005)
Abazajian, Kevork, Adelman-McCarthy, Jennifer K., Agüeros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., ...
This paper describes the Third Data Release of the Sloan Digital Sky Survey (SDSS). This release, containing data taken up through 2003 June, includes imaging data in five bands over 5282 deg2,...
Ashley, Michael C., Bailey, Jeremy A., Bedding, Timothy R., Blake, Christopher J., Bland-Hawthorn, Jonathan, Bond, I. A., ...
The cold, dry, and stable air above the summits of the Antarctic plateau provides the best ground-based observing conditions from optical to sub-millimetre wavelengths to be found on the Earth....
Burton, Michael G., Lawrence, J. S., Ashley, M. C. B., Bailey, J. A., Blake, Chris, Bedding, T. R., ...
The cold, dry, and stable air above the summits of the Antarctic plateau provides the best ground-based observing conditions from optical to sub-millimetre wavelengths to be found on the Earth....
Ashley, Michael C., Bailey, Jeremy A., Bedding, Timothy R., Blake, Christopher J., Bland-Hawthorn, Jonathan, Bond, I. A., ...
The cold, dry, and stable air above the summits of the Antarctic plateau provides the best ground-based observing conditions from optical to sub-millimetre wavelengths to be found on the Earth....
Ashley, Michael C., Bailey, Jeremy A., Bedding, Timothy R., Blake, Christopher J., Bland-Hawthorn, Jonathan, Bond, I. A., ...
The cold, dry, and stable air above the summits of the Antarctic plateau provides the best ground-based observing conditions from optical to sub-millimetre wavelengths to be found on the Earth....
The color selection of quasars from redshifts 5 to 10: cloning and discovery (2005)
Chiu, Kuenley, Zheng, Wei Yan, Schneider, Donald P., Glazebrook, Karl, Iye, Masanori, Kashikawa, Nobunari, ...
We present simulations of quasar colors, magnitudes, and numbers at redshifts 5 < z < 10 based on our discovery of 10 new high-redshift quasars and the cloning of lower redshift Sloan Digital...
Cosmic star formation history and its dependence on galaxy stellar mass (2005)
Juneau, Stephanie, Glazebrook, Karl, Crampton, David, McCarthy, Patrick J., Savaglio, Sandra, Abraham, Roberto G., ...
Abstract not available.
Hilton, Matt, Collins, Chris A., De Propris, Roberto, Baldry, Ivan K., Baugh, Carlton, Bland-Hawthorn, Joss, ...
The ROSAT-European Southern Observatory (ESO) flux-limited X-ray (REFLEX) galaxy cluster survey and the Two-degree Field Galaxy Redshift Survey (2dFGRS), respectively, comprise the largest,...
Cole, Shaun, Percival, Will, Peacock, John A., Norberg, Peder, Baugh, Carlton, Frenk, Carlos S., ...
We present a power-spectrum analysis of the final 2dF Galaxy Redshift Survey (2dFGRS), employing a direct Fourier method. The sample used comprises 221 414 galaxies with measured redshifts. We...
Glazebrook, Karl, Blake, Chris
We use Monte Carlo techniques to simulate the ability of future large high-redshift galaxy surveys to measure the temporal evolution of the dark energy equation of state ω(z) , using the...
Monster redshift surveys through dispersive slitless imaging: the Baryon Oscillation Probe (2005)
Glazebrook, Karl, Baldry, Ivan K., Moos, H. Warren, Kruk, Jeffrey W., McCandliss, Stephan Robert
Wide-field imaging from space should not forget the dispersive dimension. We consider the capability of space-based imaging with a slitless grism: because of the low near-infrared background in space...
Conway, Edward, Maddox, Stephen J., Wild, Vivienne, Peacock, John A., Hawkins, Edward, Norberg, P., ...
We present an analysis of the relative bias between early- and late-type galaxies in the Two-degree Field Galaxy Redshift Survey (2dFGRS) – as defined by the η parameter of Madgwick et al., which...
The third data release of the Sloan Digital Sky Survey (2005)
Abazajian, Kevork N., Adelman-McCarthy, Jennifer K., Agueros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., ...
This paper describes the Third Data Release of the Sloan Digital Sky Survey (SDSS). This release, containing data taken up through 2003 June, includes imaging data in five bands over 5282 deg²,...
The color selection of quasars from redshifts 5 to 10: cloning and discovery (2005)
Chiu, Kuenley, Zheng, Wei Yan, Schneider, Donald P., Glazebrook, Karl, Iye, Masanori, Kashikawa, Nobunari, ...
We present simulations of quasar colors, magnitudes, and numbers at redshifts 5 < z < 10 based on our discovery of 10 new high-redshift quasars and the cloning of lower redshift Sloan Digital...
Cosmic star formation history and its dependence on galaxy stellar mass (2005)
Juneau, Stephanie, Glazebrook, Karl, Crampton, David, McCarthy, Patrick J., Savaglio, Sandra, Abraham, Roberto G., ...
Abstract not available.
Hilton, Matt, Collins, Chris A., De Propris, Roberto, Baldry, Ivan K., Baugh, Carlton, Bland-Hawthorn, Joss, ...
The ROSAT-European Southern Observatory (ESO) flux-limited X-ray (REFLEX) galaxy cluster survey and the Two-degree Field Galaxy Redshift Survey (2dFGRS), respectively, comprise the largest,...
Cole, Shaun, Percival, Will, Peacock, John A., Norberg, Peder, Baugh, Carlton, Frenk, Carlos S., ...
We present a power-spectrum analysis of the final 2dF Galaxy Redshift Survey (2dFGRS), employing a direct Fourier method. The sample used comprises 221 414 galaxies with measured redshifts. We...
Glazebrook, Karl, Blake, Chris
We use Monte Carlo techniques to simulate the ability of future large high-redshift galaxy surveys to measure the temporal evolution of the dark energy equation of state ω(z) , using the...
Monster redshift surveys through dispersive slitless imaging: the Baryon Oscillation Probe (2005)
Glazebrook, Karl, Baldry, Ivan K., Moos, H. Warren, Kruk, Jeffrey W., McCandliss, Stephan Robert
Wide-field imaging from space should not forget the dispersive dimension. We consider the capability of space-based imaging with a slitless grism: because of the low near-infrared background in space...
Conway, Edward, Maddox, Stephen J., Wild, Vivienne, Peacock, John A., Hawkins, Edward, Norberg, P., ...
We present an analysis of the relative bias between early- and late-type galaxies in the Two-degree Field Galaxy Redshift Survey (2dFGRS) – as defined by the η parameter of Madgwick et...
The third data release of the Sloan Digital Sky Survey (2005)
Abazajian, Kevork N., Adelman-McCarthy, Jennifer K., Agueros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., ...
This paper describes the Third Data Release of the Sloan Digital Sky Survey (SDSS). This release, containing data taken up through 2003 June, includes imaging data in five bands over 5282 deg²,...
Eisenstein, Daniel J., Zehavi, Idit, Hogg, David W., Scoccimarro, Roman, Blanton, Michael R., Nichol, Robert C., ...
Abstract not available.
The Gemini Deep Deep Survey, VII: the redshift evolution of the mass-metallicity relation (2005)
Savaglio, Sandra, Glazebrook, Karl, Le Borgne, Damien, Juneau, Stephanie, Abraham, Roberto G., Chen, Hsiao Wen, ...
We have investigated the mass-metallicity (M-Z) relation using galaxies at 0.4 < z <1.0 from the Gemini Deep Deep Survey (GDDS) and Canada-France Redshift Survey (CFRS). Deep K- and z-band...
The 2dF Galaxy Redshift Survey: stochastic relative biasing between galaxy populations (2005)
Wild, Vivienne, Peacock, John A., Lahav, Ofer, Conway, Edward, Maddox, Stephen J., Baldry, Ivan K., ...
It is well known that the clustering of galaxies depends on galaxy type. Such relative bias complicates the inference of cosmological parameters from galaxy redshift surveys, and is a challenge to...
The 2dF Galaxy Redshift Survey: luminosity functions by density environment and galaxy type (2005)
Croton, Darren J., Farrar, Glennys R., Norberg, Peder, Colless, Matthew, Peacock, John A., Baldry, Ivan K., ...
We use the 2dF Galaxy Redshift Survey to measure the dependence of the bJ-band galaxy luminosity function on large-scale environment, defined by density contrast in spheres of radius 8 h−1 Mpc ,...
The Sloan Digital Sky Survey u-band galaxy survey: luminosity functions and evolution (2005)
Baldry, Ivan K., Glazebrook, Karl, Budavari, Tamas, Eisenstein, Daniel J., Annis, James, Bahcall, Neta A., ...
We construct and analyse a u-band selected galaxy sample from the Sloan Digital Sky Survey (SDSS) Southern Survey, which covers 275 deg 2. The sample includes 43 223 galaxies with spectroscopic...
Eisenstein, Daniel J., Zehavi, Idit, Hogg, David W., Scoccimarro, Roman, Blanton, Michael R., Nichol, Robert C., ...
Abstract not available.
The Gemini Deep Deep Survey, VII: the redshift evolution of the mass-metallicity relation (2005)
Savaglio, Sandra, Glazebrook, Karl, Le Borgne, Damien, Juneau, Stephanie, Abraham, Roberto G., Chen, Hsiao Wen, ...
We have investigated the mass-metallicity (M-Z) relation using galaxies at 0.4 < z <1.0 from the Gemini Deep Deep Survey (GDDS) and Canada-France Redshift Survey (CFRS). Deep K- and z-band...
The 2dF Galaxy Redshift Survey: stochastic relative biasing between galaxy populations (2005)
Wild, Vivienne, Peacock, John A., Lahav, Ofer, Conway, Edward, Maddox, Steve, Baldry, Ivan K., ...
It is well known that the clustering of galaxies depends on galaxy type. Such relative bias complicates the inference of cosmological parameters from galaxy redshift surveys, and is a challenge to...
The 2dF Galaxy Redshift Survey: luminosity functions by density environment and galaxy type (2005)
Croton, Darren J., Farrar, Glennys R., Norberg, Peder, Colless, Matthew, Peacock, John A., Baldry, Ivan K., ...
We use the 2dF Galaxy Redshift Survey to measure the dependence of the bJ-band galaxy luminosity function on large-scale environment, defined by density contrast in spheres of radius 8 h−1 Mpc...
The Sloan Digital Sky Survey u-band galaxy survey: luminosity functions and evolution (2005)
Baldry, Ivan K., Glazebrook, Karl, Budavari, Tamas, Eisenstein, Daniel J., Annis, James, Bahcall, Neta A., ...
We construct and analyse a u-band selected galaxy sample from the Sloan Digital Sky Survey (SDSS) Southern Survey, which covers 275 deg 2. The sample includes 43 223 galaxies with spectroscopic...
Karl Glazebrook, Aprajita Verma, Brian Boyle, Sebastian Oliver, Robert G. Mann, Davienne Monbleau
We present a deep photometric (B- and R-band) catalog and an associated spectroscopic redshift survey conducted in the vicinity of the Hubble Deep Field–South. The spectroscopy yields 53...
Large-scale structure from 2dFGRS (2005)
Peacock, John A., Colless, Matthew, Baldry, Ivan K., Baugh, Carlton, Bland-Hawthorn, Joss, Bridges, Terry J., ...
The 2dF Galaxy Redshift Survey was the first to observe more than 100,000 redshifts, making possible precise measurements of many aspects of galaxy clustering. The final database of more than 230,000...
Burton, Michael G., Lawrence, J. S., Ashley, M. C. B., Bailey, J. A., Blake, Chris, Bedding, T. R., ...
The cold, dry, and stable air above the summits of the Antarctic plateau provides the best ground-based observing conditions from optical to sub-millimetre wavelengths to be found on the Earth....
The color selection of quasars from redshifts 5 to 10: cloning and discovery (2005)
Chiu, Kuenley, Zheng, Wei Yan, Schneider, Donald P., Glazebrook, Karl, Iye, Masanori, Kashikawa, Nobunari, ...
We present simulations of quasar colors, magnitudes, and numbers at redshifts 5 < z < 10 based on our discovery of 10 new high-redshift quasars and the cloning of lower redshift Sloan Digital...
Cosmic star formation history and its dependence on galaxy stellar mass (2005)
Juneau, Stephanie, Glazebrook, Karl, Crampton, David, McCarthy, Patrick J., Savaglio, Sandra, Abraham, Roberto G., ...
Abstract not available.
Hilton, Matt, Collins, Chris A., De Propris, Roberto, Baldry, Ivan K., Baugh, Carlton, Bland-Hawthorn, Joss, ...
The ROSAT-European Southern Observatory (ESO) flux-limited X-ray (REFLEX) galaxy cluster survey and the Two-degree Field Galaxy Redshift Survey (2dFGRS), respectively, comprise the largest,...
Cole, Shaun, Percival, Will, Peacock, John A., Norberg, Peder, Baugh, Carlton, Frenk, Carlos S., ...
We present a power-spectrum analysis of the final 2dF Galaxy Redshift Survey (2dFGRS), employing a direct Fourier method. The sample used comprises 221 414 galaxies with measured redshifts. We...
Glazebrook, Karl, Blake, Chris
We use Monte Carlo techniques to simulate the ability of future large high-redshift galaxy surveys to measure the temporal evolution of the dark energy equation of state ω(z) , using the...
Monster redshift surveys through dispersive slitless imaging: the Baryon Oscillation Probe (2005)
Glazebrook, Karl, Baldry, Ivan K., Moos, H. Warren, Kruk, Jeffrey W., McCandliss, Stephan Robert
Wide-field imaging from space should not forget the dispersive dimension. We consider the capability of space-based imaging with a slitless grism: because of the low near-infrared background in space...
Conway, Edward, Maddox, Stephen J., Wild, Vivienne, Peacock, John A., Hawkins, Edward, Norberg, P., ...
We present an analysis of the relative bias between early- and late-type galaxies in the Two-degree Field Galaxy Redshift Survey (2dFGRS) – as defined by the η parameter of Madgwick et al., which...
The third data release of the Sloan Digital Sky Survey (2005)
Abazajian, Kevork N., Adelman-McCarthy, Jennifer K., Agueros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., ...
This paper describes the Third Data Release of the Sloan Digital Sky Survey (SDSS). This release, containing data taken up through 2003 June, includes imaging data in five bands over 5282 deg²,...
Eisenstein, Daniel J., Zehavi, Idit, Hogg, David W., Scoccimarro, Roman, Blanton, Michael R., Nichol, Robert C., ...
Abstract not available.
The Gemini Deep Deep Survey, VII: the redshift evolution of the mass-metallicity relation (2005)
Savaglio, Sandra, Glazebrook, Karl, Le Borgne, Damien, Juneau, Stephanie, Abraham, Roberto G., Chen, Hsiao Wen, ...
We have investigated the mass-metallicity (M-Z) relation using galaxies at 0.4 < z <1.0 from the Gemini Deep Deep Survey (GDDS) and Canada-France Redshift Survey (CFRS). Deep K- and z-band...
The 2dF Galaxy Redshift Survey: stochastic relative biasing between galaxy populations (2005)
Wild, Vivienne, Peacock, John A., Lahav, Ofer, Conway, Edward, Maddox, Stephen J., Baldry, Ivan K., ...
It is well known that the clustering of galaxies depends on galaxy type. Such relative bias complicates the inference of cosmological parameters from galaxy redshift surveys, and is a challenge to...
The 2dF Galaxy Redshift Survey: luminosity functions by density environment and galaxy type (2005)
Croton, Darren J., Farrar, Glennys R., Norberg, Peder, Colless, Matthew, Peacock, John A., Baldry, Ivan K., ...
We use the 2dF Galaxy Redshift Survey to measure the dependence of the bJ-band galaxy luminosity function on large-scale environment, defined by density contrast in spheres of radius 8 h−1 Mpc ,...
The Sloan Digital Sky Survey u-band galaxy survey: luminosity functions and evolution (2005)
Baldry, Ivan K., Glazebrook, Karl, Budavari, Tamas, Eisenstein, Daniel J., Annis, James, Bahcall, Neta A., ...
We construct and analyse a u-band selected galaxy sample from the Sloan Digital Sky Survey (SDSS) Southern Survey, which covers 275 deg 2. The sample includes 43 223 galaxies with spectroscopic...
Large-scale structure from 2dFGRS (2005)
Peacock, John A., Colless, Matthew, Baldry, Ivan K., Baugh, Carlton, Bland-Hawthorn, Joss, Bridges, Terry J., ...
The 2dF Galaxy Redshift Survey was the first to observe more than 100,000 redshifts, making possible precise measurements of many aspects of galaxy clustering. The final database of more than 230,000...
Monster Redshift Surveys through Dispersive Slitless Imaging: The Baryon Oscillation Probe (2004)
Glazebrook, Karl, Baldry, Ivan, Moos, Warren, Kruk, Jeff, McCandliss, Stephan
Wide-field imaging from space should not forget the dispersive dimension. We consider the capability of space-based imaging with a slitless grism: because of the low near-infrared background in space...
The 2dF Galaxy Redshift Survey: the local E+A galaxy population (2004)
Blake, Chris, Pracy, Michael, Couch, Warrick, Bekki, Kenji, Lewis, Ian, Glazebrook, Karl, ...
We select a sample of low-redshift (z ~ 0.1) E+A galaxies from the 2dF Galaxy Redshift Survey (2dFGRS). The spectra of these objects are defined by strong hydrogen Balmer absorption lines (H-delta,...
Glazebrook, Karl, Tober, Jeffrey, Thomson, Scott, Bland-Hawthorn, Joss, Abraham, Roberto
We report the results of a deep 3D imaging survey of the Hubble Deep Field North using the Taurus Tunable Filter and the William Herschel Telescope. This survey was designed to search for new line...
FORTIS: Pathfinder to the Lyman Continuum (2004)
McCandliss, Stephan R., France, Kevin, Feldman, Paul D., Glazebrook, Karl, Meurer, Gerhardt, Bianchi, Luciana, ...
Shull et al. (1999) have asserted that the contribution of stars, relative to quasars, to the metagalactic background radiation that ionizes most of the baryons in the universe remains almost...
Percival, Will J., Burkey, Daniel, Heavens, Alan, Taylor, Andy, Cole, Shaun, Peacock, John A., ...
We present the result of a decomposition of the 2dFGRS galaxy overdensity field into an orthonormal basis of spherical harmonics and spherical Bessel functions. Galaxies are expected to directly...
The bimodal galaxy color distribution: dependence on luminosity and environment (2004)
Balogh, Michael L., Baldry, Ivan K., Nichol, Robert, Miller, Chris, Bower, Richard, Glazebrook, Karl
We analyse the u-r color distribution of 24346 galaxies with Mr
Substructure Analysis of Selected Low Richness 2dFGRS Clusters of Galaxies (2004)
Burgett, William S., Vick, Michael M., Davis, David S., Colless, Matthew, De Propris, Roberto, Baldry, Ivan, ...
Complementary one-, two-, and three-dimensional tests for detecting the presence of substructure in clusters of galaxies are applied to recently obtained data from the 2dF Galaxy Redshift Survey. The...
De Propris, Roberto, Colless, Matthew, Peacock, John, Couch, Warrick, Driver, Simon, Balogh, Michael, ...
We derive the fraction of blue galaxies in a sample of clusters at z < 0.11 and the general field at the same redshift. The value of the blue fraction is observed to depend on the luminosity limit...
The Gemini Deep Deep Survey: I. Introduction to the Survey, Catalogs and Composite Spectra (2004)
Abraham, Roberto G., Glazebrook, Karl, McCarthy, Patrick J., Crampton, David, Murowinski, Richard, Jorgensen, Inger, ...
The Gemini Deep Deep Survey (GDDS) is an ultra-deep (K
Norman, Colin, Ptak, Andrew, Hornschemeier, Ann, Hasinger, Guenther, Bergeron, Jacqueline, Comastri, Andrea, ...
The cosmological star formation rate in the combined Chandra Deep Fields North and South is derived from our X-Ray Luminosity Function for Galaxies in these Deep Fields. Mild evolution is seen up to...
Glazebrook, Karl, Abraham, Roberto, McCarthy, Patrick, Savaglio, Sandra, Chen, Hsiao-Wen, Crampton, David, ...
Hierarchical galaxy formation is the model whereby massive galaxies form from an assembly of smaller units. The most massive objects therefore form last. The model succeeds in describing the...
The 2dF Galaxy Redshift Survey: the clustering of galaxy groups (2004)
Padilla, Nelson D., Baugh, Carlton M., Eke, Vincent R., Norberg, Peder, Cole, Shaun, Frenk, Carlos S., ...
The second data release of the Sloan Digital Sky Survey (2004)
Abazajian, Kevork, Adelman-McCarthy, Jennifer K., Agüeros, Marcel A., Allam, Sahar S., Anderson, Kurt, Anderson, Scott F., ...
The Sloan Digital Sky Survey (SDSS) has validated and made publicly available its Second Data Release. This data release consists of 3324 deg2 of five-band (ugriz) imaging data with photometry for...
Substructure analysis of selected low-richness 2dFGRS clusters of galaxies (2004)
Burgett, William S., Vick, Michael M., Davis, D. Scott, Colless, Matthew, De Propris, Roberto, Baldry, Ivan K., ...
Complementary one-, two- and three-dimensional tests for detecting the presence of substructure in clusters of galaxies are applied to recently obtained data from the 2dF Galaxy Redshift Survey. The...
Galaxy ecology : groups and low-density environments in the SDSS and 2dFGRS (2004)
Balogh, Michael L., Eke, Vince, Miller, Christopher J., Lewis, Ian, Bower, Richard G., Couch, Warrick J., ...
We analyse the observed correlation between galaxy environment and Hα emission-line strength, using volume-limited samples and group catalogues of 24 968 galaxies at 0.05 < z < 0.095,...
The Gemini Deep Deep Survey I: introduction to the survey, catalogs, and composite spectra (2004)
Abraham, Roberto G., Glazebrook, Karl, McCarthy, Patrick J., Crampton, David, Murowinski, Richard, Jorgensen, Inger, ...
The Gemini Deep Deep Survey (GDDS) is an ultradeep (K < 20.6 mag, I < 24.5 mag) redshift survey targeting galaxies in the "redshift desert" between z = 1 and z = 2. The primary goal of the...
Eke, Vince, Frenk, Carlos S., Baugh, Carlton, Cole, Shaun, Norberg, Peder, Peacock, John A., ...
The Two-degree Field Galaxy Redshift Survey (2dFGRS) Percolation-Inferred Galaxy Group (2PIGG) catalogue of ∼29 000 objects is used to study the luminous content of galaxy systems of various...
Norman, Colin, Ptak, Andrew F., Hornschemeier, Ann, Hasinger, Gunther H., Bergeron, Jacqueline, Comastri, Andrea, ...
The cosmological star formation rate in the combined Chandra Deep Fields North and South is derived from our X-ray luminosity function for galaxies in these deep fields. Mild evolution is seen up to...
A Ly alpha-only active galactic nucleus from the Sloan Digital Sky Survey (2004)
Hall, Patrick B., Hoversten, E. A., Tremonti, Christy A., Vanden Berk, Daniel E., Schneider, Donald P., Strauss, Michael A., ...
The Sloan Digital Sky Survey has discovered a z = 2.4917 radio-loud active galactic nucleus (AGN) with a luminous, variable, low-polarization UV continuum, H I two-photon emission, and a moderately...
Galaxy groups in the 2dFGRS: the group-finding algorithm and the 2PIGG catalogue (2004)
Eke, Vince, Baugh, Carlton, Cole, Shaun, Frenk, Carlos S., Norberg, Peder, Peacock, John A., ...
The construction of a catalogue of galaxy groups from the Two-degree Field Galaxy Redshift Survey (2dFGRS) is described. Groups are identified by means of a friends-of-friends percolation algorithm...
Glazebrook, Karl, Tober, Jeffrey, Thomson, Scott, Bland-Hawthorn, Joss, Abraham, Roberto G.
We report the results of a deep three-dimensional imaging survey of the Hubble Deep Field North using the Taurus Tunable Filter at the William Herschel Telescope. This survey was designed to search...
The 2dF Galaxy Redshift Survey: the local E+A galaxy population (2004)
Blake, Chris, Pracy, Michael B., Couch, Warrick J., Bekki, Kenji, Lewis, Ian, Glazebrook, Karl, ...
We select a sample of low-redshift (z ∼ 0.1) E+A galaxies from the 2dF Galaxy Redshift Survey (2dFGRS). The spectra of these objects are defined by strong hydrogen Balmer absorption lines...
The second data release of the Sloan Digital Sky Survey (2004)
Abazajian, Kevork N., Adelman-McCarthy, Jennifer K., Agueros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., ...
The Sloan Digital Sky Survey (SDSS) has validated and made publicly available its Second Data Release. This data release consists of 3324 deg(2) of five-band (ugriz) imaging data with photometry for...
The 2dF Galaxy Redshift Survey: the clustering of galaxy groups (2004)
Padilla, Nelson D., Baugh, Carlton, Eke, Vincent R., Norberg, Peder, Cole, Shaun, Frenk, Carlos S., ...
We measure the clustering of galaxy groups in the 2dFGRS Percolation-Inferred Galaxy Group (2PIGG) catalogue. The 2PIGG sample has 28 877 groups with at least two members. The clustering amplitude of...
De Propris, Roberto, Colless, Matthew, Peacock, John A., Couch, Warrick J., Driver, Simon P., Balogh, Michael L., ...
We derive the fraction of blue galaxies in a sample of clusters at z < 0.11 and the general field at the same redshift. The value of the blue fraction is observed to depend on the luminosity limit...
Quantifying the bimodal color-magnitude distribution of galaxies (2004)
Baldry, Ivan K., Glazebrook, Karl, Brinkmann, Jon, Ivezic, Zeljko, Lupton, Robert H., Nichol, Robert C., ...
We analyze the bivariate distribution, in color versus absolute magnitude (u-r vs. Mr), of a low-redshift sample of galaxies from the Sloan Digital Sky Survey (2400 deg2, 0.004 < z < 0.08,...
The 2dF Galaxy Redshift Survey: higher-order galaxy correlation functions (2004)
Croton, Darren J., Gaztanaga, Enrique, Baugh, Carlton, Norberg, Peder, Colless, Matthew, Baldry, Ivan K., ...
We measure moments of the galaxy count probability distribution function in the Two-degree Field Galaxy Redshift Survey (2dFGRS). The survey is divided into volume-limited subsamples in order to...
The 2dF Galaxy Redshift Survey: Wiener reconstruction of the cosmic web (2004)
Erdogdu, Pirin, Lahav, Ofer, Zaroubi, Saleem, Efstathiou, George P., Moody, Stephen J., Peacock, John A., ...
We reconstruct the underlying density field of the Two-degree Field Galaxy Redshift Survey (2dFGRS) for the redshift range 0.035 < z < 0.200 using the Wiener filtering method. The Wiener filter...
L ' and M ' photometry of ultracool dwarfs (2004)
Golimowski, David A., Leggett, Sandy K., Marley, Mark S., Fan, Xiaohui, Geballe, Thomas R., Knapp, Gillian R., ...
We have compiled L′ (3.4-4.1 μm) and M′ (4.6-4.8 μm) photometry of 63 single and binary M, L, and T dwarfs obtained at the United Kingdom Infrared Telescope using the Mauna...
Selection and photometric properties of K+A galaxies (2004)
Quintero, Alejandro D., Hogg, David W., Blanton, Michael R., Schlegel, David J., Eisenstein, Daniel J., Gunn, James E., ...
Two different simple measurements of galaxy star formation rate with different timescales are compared empirically on 156,395 fiber spectra of galaxies with r < 17.77 mag taken from the Sloan...
Savaglio, Sandra, Glazebrook, Karl, Abraham, Roberto G., Crampton, David, Chen, Hsiao-Wen, McCarthy, Patrick J., ...
The goal of the Gemini Deep Deep Survey (GDDS) is to study an unbiased sample of K < 20.6 galaxies in the redshift range 0.8 < z < 2.0. Here we determine the statistical properties of the...
Knapp, Gillian R., Leggett, Sandy K., Fan, Xiaohui, Marley, Mark S., Geballe, Thomas R., Golimowski, David A., ...
We present new JHK photometry on the MKO-NIR system and JHK spectroscopy for a large sample of L and T dwarfs. Photometry has been obtained for 71 dwarfs, and spectroscopy for 56. The sample...
McCarthy, Patrick J., Le Borgne, Damien, Crampton, David, Chen, Hsiao-Wen, Abraham, Roberto G., Glazebrook, Karl, ...
We present spectroscopic evidence from the Gemini Deep Deep Survey for a significant population of color-selected red galaxies at 1.3 < z, < 2.2 whose integrated light is dominated by evolved...
Three Ly alpha emitters at z ≈ 6: early GMOS/Gemini data from the GLARE project (2004)
Stanway, Elizabeth R., Glazebrook, Karl, Bunker, Andrew J., Abraham, R. G., Hook, Isobel, Rhoads, James, ...
We report spectroscopic detection of three z ∼ 6 Lyα-emitting galaxies, in the vicinity of the Hubble Ultra Deep Field, from the early data of the Gemini Lyman Alpha at Reionisation Era...
The 2dF Galaxy Redshift Survey: hierarchical galaxy clustering (2004)
Baugh, Carlton, Croton, Darren J., Gaztanaga, Enrique, Norberg, Peder, Colless, Matthew, Baldry, Ivan K., ...
We use the Two-Degree Field Galaxy Redshift Survey (2dFGRS) to test the hierarchical scaling hypothesis: namely, that the p-point galaxy correlation functions can be written in terms of the two-point...
The bimodal galaxy color distribution: dependence on luminosity and environment (2004)
Balogh, Michael L., Baldry, Ivan K., Nichol, Robert C., Miller, Christopher J., Bower, Richard G., Glazebrook, Karl
We analyze the u - r color distribution of 24,346 galaxies with M r ≤ -18 and z < 0.08, drawn from the Sloan Digital Sky Survey first data release, as a function of luminosity and...
The 2dF Galaxy Redshift Survey: voids and hierarchical scaling models (2004)
Croton, Darren J., Colless, Matthew, Gaztanaga, Enrique, Baugh, Carlton, Norberg, Peder, Baldry, Ivan K., ...
We measure the redshift-space reduced void probability function (VPF) for 2dFGRS volume-limited galaxy samples covering the absolute magnitude range MbJ -5log10 h = -18 to -22. Theoretically, the VPF...
Percival, Will J., Burkey, Daniel, Heavens, Alan F., Taylor, Andy N., Cole, Shaun, Peacock, John A., ...
We present the result of a decomposition of the 2dF Galaxy Redshift Survey (2dFGRS) galaxy overdensity field into an orthonormal basis of spherical harmonics and spherical Bessel functions. Galaxies...
The 2dF galaxy redshift survey: clustering properties of radio galaxies (2004)
Magliocchetti, Manuela, Maddox, Stephen J., Hawkins, Edward, Peacock, John A., Bland-Hawthorn, Joss, Bridges, Terry J., ...
The clustering properties of local, S1.4 GHz ≥ 1 mJy, radio sources are investigated for a sample of 820 objects drawn from the joint use of the Faint Images of the Radio Sky at 20 cm (FIRST)...
A high abundance of massive galaxies 3-6 billion years after the Big Bang (2004)
Glazebrook, Karl, Abraham, Roberto G., McCarthy, Patrick J., Savaglio, Sandra, Chen, Hsiao-Wen, Crampton, David, ...
Hierarchical galaxy formation is the model whereby massive galaxies form from an assembly of smaller units. The most massive objects therefore form last. The model succeeds in describing the...
FORTIS: pathfinder to the lyman continuum (2004)
McCandliss, Stephan R., France, Kevin, Feldman, Paul D., Glazebrook, Karl, Meurer, Gerhardt, Blanchi, Luciana, ...
Abstract not reproduced here by request of the publisher. The text is available from: http://dx.doi.org/10.1117/12.552799.
Substructure analysis of selected low-richness 2dFGRS clusters of galaxies (2004)
Burgett, William S., Vick, Michael M., Davis, David S., Colless, Matthew, De Propris, Roberto, Baldry, Ivan, ...
Complementary one-, two- and three-dimensional tests for detecting the presence of substructure in clusters of galaxies are applied to recently obtained data from the 2dF Galaxy Redshift Survey. The...
Galaxy ecology: groups and low-density environments in the SDSS and 2dFGRS (2004)
Balogh, Michael L., Eke, Vince, Miller, Christopher J., Lewis, Ian, Bower, Richard G., Couch, Warrick J., ...
We analyse the observed correlation between galaxy environment and Hα emission-line strength, using volume-limited samples and group catalogues of 24 968 galaxies at 0.05 < z < 0.095, drawn from the...
The Gemini Deep Deep Survey I: introduction to the survey, catalogs, and composite spectra (2004)
Abraham, Roberto G., Glazebrook, Karl, McCarthy, Patrick J., Crampton, David, Murowinski, Richard, Jorgensen, Inger, ...
The Gemini Deep Deep Survey (GDDS) is an ultradeep (K < 20.6 mag, I < 24.5 mag) redshift survey targeting galaxies in the "redshift desert" between z = 1 and z = 2. The primary goal of the...
Eke, Vince, Frenk, Carlos S., Baugh, Carlton, Cole, Shaun, Norberg, Peder, Peacock, John A., ...
The Two-degree Field Galaxy Redshift Survey (2dFGRS) Percolation-Inferred Galaxy Group (2PIGG) catalogue of ∼29 000 objects is used to study the luminous content of galaxy systems of various...
Norman, Colin, Ptak, Andrew F., Hornschemeier, Ann, Hasinger, Gunther H., Bergeron, Jacqueline, Comastri, Andrea, ...
The cosmological star formation rate in the combined Chandra Deep Fields North and South is derived from our X-ray luminosity function for galaxies in these deep fields. Mild evolution is seen up to...
A Ly alpha-only active galactic nucleus from the Sloan Digital Sky Survey (2004)
Hall, Patrick B., Hoversten, E. A., Tremonti, Christy A., Vanden Berk, Daniel E., Schneider, Donald P., Strauss, Michael A., ...
The Sloan Digital Sky Survey has discovered a z = 2.4917 radio-loud active galactic nucleus (AGN) with a luminous, variable, low-polarization UV continuum, H I two-photon emission, and a moderately...
Galaxy groups in the 2dFGRS: the group-finding algorithm and the 2PIGG catalogue (2004)
Eke, Vince, Baugh, Carlton, Cole, Shaun, Frenk, Carlos S., Norberg, Peder, Peacock, John A., ...
The construction of a catalogue of galaxy groups from the Two-degree Field Galaxy Redshift Survey (2dFGRS) is described. Groups are identified by means of a friends-of-friends percolation algorithm...
Glazebrook, Karl, Tober, Jeffrey, Thomson, Scott, Bland-Hawthorn, Joss, Abraham, Roberto G.
We report the results of a deep three-dimensional imaging survey of the Hubble Deep Field North using the Taurus Tunable Filter at the William Herschel Telescope. This survey was designed to search...
The 2dF Galaxy Redshift Survey: the local E+A galaxy population (2004)
Blake, Chris, Pracy, Michael B., Couch, Warrick J., Bekki, Kenji, Lewis, Ian, Glazebrook, Karl, ...
We select a sample of low-redshift (z ∼ 0.1) E+A galaxies from the 2dF Galaxy Redshift Survey (2dFGRS). The spectra of these objects are defined by strong hydrogen Balmer absorption lines...
The second data release of the Sloan Digital Sky Survey (2004)
Abazajian, Kevork N., Adelman-McCarthy, Jennifer K., Agueros, Marcel A., Allam, Sahar S., Anderson, Kurt S. J., Anderson, Scott F., ...
The Sloan Digital Sky Survey (SDSS) has validated and made publicly available its Second Data Release. This data release consists of 3324 deg(2) of five-band (ugriz) imaging data with photometry for...
The 2dF Galaxy Redshift Survey: the clustering of galaxy groups (2004)
Padilla, Nelson D., Baugh, Carlton, Eke, Vincent R., Norberg, Peder, Cole, Shaun, Frenk, Carlos S., ...
We measure the clustering of galaxy groups in the 2dFGRS Percolation-Inferred Galaxy Group (2PIGG) catalogue. The 2PIGG sample has 28 877 groups with at least two members. The clustering amplitude of...
De Propris, Roberto, Colless, Matthew, Peacock, John A., Couch, Warrick J., Driver, Simon P., Balogh, Michael L., ...
We derive the fraction of blue galaxies in a sample of clusters at z < 0.11 and the general field at the same redshift. The value of the blue fraction is observed to depend on the luminosity limit...
Quantifying the bimodal color-magnitude distribution of galaxies (2004)
Baldry, Ivan K., Glazebrook, Karl, Brinkmann, Jon, Ivezic, Zeljko, Lupton, Robert H., Nichol, Robert C., ...
We analyze the bivariate distribution, in color versus absolute magnitude (u-r vs. Mr), of a low-redshift sample of galaxies from the Sloan Digital Sky Survey (2400 deg2, 0.004 < z < 0.08,...
The 2dF Galaxy Redshift Survey: higher-order galaxy correlation functions (2004)
Croton, Darren J., Gaztanaga, Enrique, Baugh, Carlton, Norberg, Peder, Colless, Matthew, Baldry, Ivan K., ...
We measure moments of the galaxy count probability distribution function in the Two-degree Field Galaxy Redshift Survey (2dFGRS). The survey is divided into volume-limited subsamples in order to...
The 2dF Galaxy Redshift Survey: Wiener reconstruction of the cosmic web (2004)
Erdogdu, Pirin, Lahav, Ofer, Zaroubi, Saleem, Efstathiou, George P., Moody, Stephen J., Peacock, John A., ...
We reconstruct the underlying density field of the Two-degree Field Galaxy Redshift Survey (2dFGRS) for the redshift range 0.035 < z < 0.200 using the Wiener filtering method. The Wiener filter...
L ' and M ' photometry of ultracool dwarfs (2004)
Golimowski, David A., Leggett, Sandy K., Marley, Mark S., Fan, Xiaohui, Geballe, Thomas R., Knapp, Gillian R., ...
We have compiled L′ (3.4-4.1 μm) and M′ (4.6-4.8 μm) photometry of 63 single and binary M, L, and T dwarfs obtained at the United Kingdom Infrared Telescope using the Mauna...
Selection and photometric properties of K+A galaxies (2004)
Quintero, Alejandro D., Hogg, David W., Blanton, Michael R., Schlegel, David J., Eisenstein, Daniel J., Gunn, James E., ...
Two different simple measurements of galaxy star formation rate with different timescales are compared empirically on 156,395 fiber spectra of galaxies with r < 17.77 mag taken from the Sloan...
Savaglio, Sandra, Glazebrook, Karl, Abraham, Roberto G., Crampton, David, Chen, Hsiao-Wen, McCarthy, Patrick J., ...
The goal of the Gemini Deep Deep Survey (GDDS) is to study an unbiased sample of K < 20.6 galaxies in the redshift range 0.8 < z < 2.0. Here we determine the statistical properties of the...
Knapp, Gillian R., Leggett, Sandy K., Fan, Xiaohui, Marley, Mark S., Geballe, Thomas R., Golimowski, David A., ...
We present new JHK photometry on the MKO-NIR system and JHK spectroscopy for a large sample of L and T dwarfs. Photometry has been obtained for 71 dwarfs, and spectroscopy for 56. The sample...
McCarthy, Patrick J., Le Borgne, Damien, Crampton, David, Chen, Hsiao-Wen, Abraham, Roberto G., Glazebrook, Karl, ...
We present spectroscopic evidence from the Gemini Deep Deep Survey for a significant population of color-selected red galaxies at 1.3 < z, < 2.2 whose integrated light is dominated by evolved...
Three Ly alpha emitters at z ≈ 6: early GMOS/Gemini data from the GLARE project (2004)
Stanway, Elizabeth R., Glazebrook, Karl, Bunker, Andrew J., Abraham, R. G., Hook, Isobel, Rhoads, James, ...
We report spectroscopic detection of three z ∼ 6 Lyα-emitting galaxies, in the vicinity of the Hubble Ultra Deep Field, from the early data of the Gemini Lyman Alpha at Reionisation Era (GLARE)...
The 2dF Galaxy Redshift Survey: hierarchical galaxy clustering (2004)
Baugh, Carlton, Croton, Darren J., Gaztanaga, Enrique, Norberg, Peder, Colless, Matthew, Baldry, Ivan K., ...
We use the Two-Degree Field Galaxy Redshift Survey (2dFGRS) to test the hierarchical scaling hypothesis: namely, that the p-point galaxy correlation functions can be written in terms of the two-point...
The bimodal galaxy color distribution: dependence on luminosity and environment (2004)
Balogh, Michael L., Baldry, Ivan K., Nichol, Robert C., Miller, Christopher J., Bower, Richard G., Glazebrook, Karl
We analyze the u - r color distribution of 24,346 galaxies with M r ≤ -18 and z < 0.08, drawn from the Sloan Digital Sky Survey first data release, as a function of luminosity and...
The 2dF Galaxy Redshift Survey: voids and hierarchical scaling models (2004)
Croton, Darren J., Colless, Matthew, Gaztanaga, Enrique, Baugh, Carlton, Norberg, Peder, Baldry, Ivan K., ...
We measure the redshift-space reduced void probability function (VPF) for 2dFGRS volume-limited galaxy samples covering the absolute magnitude range MbJ -5log10 h = -18 to -22. Theoretically, the VPF...
Percival, Will J., Burkey, Daniel, Heavens, Alan F., Taylor, Andy N., Cole, Shaun, Peacock, John A., ...
We present the result of a decomposition of the 2dF Galaxy Redshift Survey (2dFGRS) galaxy overdensity field into an orthonormal basis of spherical harmonics and spherical Bessel functions. Galaxies...
The 2dF Galaxy Redshift Survey: clustering properties of radio galaxies (2004)
Magliocchetti, Manuela, Maddox, Stephen J., Hawkins, Edward, Peacock, John A., Bland-Hawthorn, Joss, Bridges, Terry J., ...
The clustering properties of local, S1.4 GHz ≥ 1 mJy, radio sources are investigated for a sample of 820 objects drawn from the joint use of the Faint Images of the Radio Sky at 20 cm (FIRST) and...
A high abundance of massive galaxies 3-6 billion years after the Big Bang (2004)
Glazebrook, Karl, Abraham, Roberto G., McCarthy, Patrick J., Savaglio, Sandra, Chen, Hsiao-Wen, Crampton, David, ...
Hierarchical galaxy formation is the model whereby massive galaxies form from an assembly of smaller units. The most massive objects therefore form last. The model succeeds in describing the...
FORTIS: pathfinder to the lyman continuum (2004)
McCandliss, Stephan R., France, Kevin, Feldman, Paul D., Glazebrook, Karl, Meurer, Gerhardt, Blanchi, Luciana, ...
Abstract not reproduced here by request of the publisher. The text is available from: http://dx.doi.org/10.1117/12.552799.
The 2dF Galaxy Redshift Survey: Wiener Reconstruction of the Cosmic Web (2003)
Erdogdu, Pirin, Lahav, Ofer, Zaroubi, Saleem, Efstathiou, George, Moody, Steve, Peacock, John A., ...
We reconstruct the underlying density field of the 2 degree Field Galaxy Redshift Survey (2dFGRS) for the redshift range 0.035
Three Lyman-alpha Emitters at z approx 6: Early GMOS/Gemini Data from the GLARE Project (2003)
Stanway, Elizabeth R., Glazebrook, Karl, Bunker, Andrew J., Abraham, Roberto G., Hook, Isobel, Rhoads, James, ...
We report spectroscopic detection of three z~6 Lyman-alpha emitting galaxies, in the vicinity of the Hubble Ultra Deep Field, from the early data of the Gemini Lyman-$\alpha$ at Reionisation Era...
The 2dF Galaxy Redshift Survey: Clustering properties of radio galaxies (2003)
Magliocchetti, Manuela, Maddox, Steve J., Hawkins, Ed, Peacock, John A., Bland-Hawthorn, Joss, Bridges, Terry, ...
The clustering properties of local, S_{1.4 GHz} > 1 mJy, radio sources are investigated for a sample of 820 objects drawn from the joint use of the FIRST and 2dF Galaxy Redshift surveys. To this aim,...
Galaxy ecology: groups and low-density environments in the SDSS and 2dFGRS (2003)
Balogh, Michael, Eke, Vince, Miller, Chris, Lewis, Ian, Bower, Richard, Couch, Warrick, ...
We analyse the observed correlation between galaxy environment and H-alpha emission line strength, using volume-limited samples and group catalogues of 24968 galaxies drawn from the 2dF Galaxy...
Glazebrook, Karl, Team, The GDDS
The aim of the Gemini Deep Deep Survey is to push spectroscopic studies of complete galaxy samples (both red and blue objects) significantly beyond z=1; this is the redshift where the current Hubble...
Selection and photometric properties of K+A galaxies (2003)
Quintero, Alejandro D., Hogg, David W., Blanton, Michael R., Schlegel, David J., Eisenstein, Daniel J., Gunn, James E., ...
Two different simple measurements of galaxy star formation rate with different timescales are compared empirically on $156,395$ fiber spectra of galaxies with $r
The 2dF Galaxy Redshift Survey: Final Data Release (2003)
Colless, Matthew, Peterson, Bruce A., Jackson, Carole, Peacock, John A., Cole, Shaun, Norberg, Peder, ...
The 2dF Galaxy Redshift Survey (2dFGRS) has obtained spectra for 245591 sources, mainly galaxies, brighter than a nominal extinction-corrected magnitude limit of b_J=19.45. Reliable redshifts were...
Blake, Chris, Glazebrook, Karl
We show that the baryonic oscillations expected in the galaxy power spectrum may be used as a "standard cosmological ruler'' to facilitate accurate measurement of the cosmological equation of state....
The 2dF Galaxy Redshift Survey: final data release (2003)
Colless, Matthew, Peterson, Bruce A., Jackson, Carole, Peacock, John A., Cole, Shaun, Norberg, Peder, ...
The 2dF Galaxy Redshift Survey (2dFGRS) has obtained spectra for 245591 sources, mainly galaxies, brighter than a nominal extinction-corrected magnitude limit of b_J=19.45. Reliable redshifts were...
The 2dF Galaxy Redshift Survey: final data release (2003)
Colless, Matthew, Peterson, Bruce A., Jackson, Carole, Peacock, John A., Cole, Shaun, Norberg, Peder, ...
The 2dF Galaxy Redshift Survey (2dFGRS) has obtained spectra for 245591 sources, mainly galaxies, brighter than a nominal extinction-corrected magnitude limit of b_J=19.45. Reliable redshifts were...
The 2dF Galaxy Redshift Survey: galaxy clustering per spectral type (2003)
Madgwick, Darren, Hawkins, Edward, Lahav, Ofer, Maddox, Stephen J., Norberg, Peder, Peacock, John A., ...
We have calculated the two-point correlation functions in redshift space, Ζ (σ, π), for galaxies of different spectral types in the 2dF Galaxy Redshift Survey. Using these...
Baldry, Ivan K., Glazebrook, Karl
We obtain constraints on the slope of a universal stellar initial mass function (IMF) over a range of model cosmic star formation histories (SFHs) using z ≈ 0.1 luminosity densities in the...
Huang, Jiasheng Sheng, Glazebrook, Karl, Cowie, Lennox L., Tinney, C.
We present the K-band local luminosity function derived from a sample of 1056 bright (K < 15) K-selected galaxies from the Hawaii+Anglo-Australian Observatory (AAO) K-band redshift survey. The...
The 2dF Galaxy Redshift Survey: the luminosity function of cluster galaxies (2003)
De Propris, Roberto, Colless, Matthew, Driver, Simon P., Couch, Warrick J., Peacock, John A., Baldry, Ivan K., ...
We have determined the composite luminosity function (LF) for galaxies in 60 clusters from the 2dF Galaxy Redshift Survey. The LF spans the range -22.5 < MbJ <-15, and is well fitted by a...
The Sloan Digital Sky Survey: the cosmic spectrum and star formation history (2003)
Glazebrook, Karl, Baldry, Ivan K., Blanton, Michael R., Brinkmann, Jon, Connolly, Andrew J., Csabai, Istvan, ...
We present a determination of the "cosmic optical spectrum" of the universe, i.e., the ensemble emission from galaxies, as determined from the red-selected Sloan Digital Sky Survey main galaxy...
Blake, Chris, Glazebrook, Karl
We show that the baryonic oscillations expected in the galaxy power spectrum may be used as a "standard cosmological ruler" to facilitate accurate measurement of the cosmological equation of state....
Hawkins, Edward, Maddox, Stephen J., Cole, Shaun, Lahav, Ofer, Madgwick, Darren, Norberg, Peder, ...
We present a detailed analysis of the two-point correlation function, ξ(σ, π) , from the 2dF Galaxy Redshift Survey (2dFGRS). The large size of the catalogue, which contains...
The first data release of the Sloan Digital Sky Survey (2003)
Abazajian, Kevork N., Adelman-McCarthy, Jennifer K., Agueros, Marcel A., Allam, Sahar S., Anderson, Scott F., Annis, James, ...
The Sloan Digital Sky Survey (SDSS) has validated and made publicly available its First Data Release. This consists of 2099 deg2 of five-band (u, g, r, i, z) imaging data, 186,240 spectra of...
The 2dF Galaxy Redshift Survey: galaxy clustering per spectral type (2003)
Madgwick, Darren, Hawkins, Edward, Lahav, Ofer, Maddox, Stephen J., Norberg, Peder, Peacock, John A., ...
We have calculated the two-point correlation functions in redshift space, Ζ (σ, π), for galaxies of different spectral types in the 2dF Galaxy Redshift Survey. Using these...
Baldry, Ivan K., Glazebrook, Karl
We obtain constraints on the slope of a universal stellar initial mass function (IMF) over a range of model cosmic star formation histories (SFHs) using z ≈ 0.1 luminosity densities in the...
Huang, Jiasheng Sheng, Glazebrook, Karl, Cowie, Lennox L., Tinney, C.
We present the K-band local luminosity function derived from a sample of 1056 bright (K < 15) K-selected galaxies from the Hawaii+Anglo-Australian Observatory (AAO) K-band redshift survey. The...
The 2dF Galaxy Redshift Survey: the luminosity function of cluster galaxies (2003)
De Propris, Roberto, Colless, Matthew, Driver, Simon P., Couch, Warrick J., Peacock, John A., Baldry, Ivan K., ...
We have determined the composite luminosity function (LF) for galaxies in 60 clusters from the 2dF Galaxy Redshift Survey. The LF spans the range -22.5 < MbJ <-15, and is well fitted by a...
The Sloan Digital Sky Survey: the cosmic spectrum and star formation history (2003)
Glazebrook, Karl, Baldry, Ivan K., Blanton, Michael R., Brinkmann, Jon, Connolly, Andrew J., Csabai, Istvan, ...
We present a determination of the "cosmic optical spectrum" of the universe, i.e., the ensemble emission from galaxies, as determined from the red-selected Sloan Digital Sky Survey main galaxy...
Blake, Chris, Glazebrook, Karl
We show that the baryonic oscillations expected in the galaxy power spectrum may be used as a "standard cosmological ruler" to facilitate accurate measurement of the cosmological equation of state....
Hawkins, Edward, Maddox, Stephen J., Cole, Shaun, Lahav, Ofer, Madgwick, Darren, Norberg, Peder, ...
We present a detailed analysis of the two-point correlation function, ξ(σ, π) , from the 2dF Galaxy Redshift Survey (2dFGRS). The large size of the catalogue, which contains...
The first data release of the Sloan Digital Sky Survey (2003)
Abazajian, Kevork N., Adelman-McCarthy, Jennifer K., Agueros, Marcel A., Allam, Sahar S., Anderson, Scott F., Annis, James, ...
The Sloan Digital Sky Survey (SDSS) has validated and made publicly available its First Data Release. This consists of 2099 deg2 of five-band (u, g, r, i, z) imaging data, 186,240 spectra of...
The 2dF Galaxy Redshift Survey: final data release (2003)
Colless, Matthew, Peterson, Bruce A., Jackson, Carole, Peacock, John A., Cole, Shaun, Norberg, Peder, ...
The 2dF Galaxy Redshift Survey (2dFGRS) has obtained spectra for 245591 sources, mainly galaxies, brighter than a nominal extinction-corrected magnitude limit of b_J=19.45. Reliable redshifts were...
The Sloan Digital Sky Survey: The Cosmic Spectrum and Star-Formation History (2002)
Glazebrook, Karl, Baldry, Ivan K., Blanton, Michael R., Brinkmann, Jon, Connolly, Andrew, Csabai, Istvan, ...
We present a determination of the `Cosmic Optical Spectrum' of the Universe, i.e. the ensemble emission from galaxies, as determined from the red-selected Sloan Digital Sky Survey main galaxy sample...
Parameter constraints for flat cosmologies from CMB and 2dFGRS power spectra (2002)
Percival, Will J., Sutherland, Will, Peacock, John A., Baugh, Carlton M., Bland-Hawthorn, Joss, Bridges, Terry, ...
We constrain flat cosmological models with a joint likelihood analysis of a new compilation of data from the cosmic microwave background (CMB) and from the 2dF Galaxy Redshift Survey (2dFGRS)....
An H-alpha survey of the rich cluster A1689 (2002)
Balogh, Michael, Couch, Warrick J., Smail, Ian, Bower, Richard G., Glazebrook, Karl
(Abridged) We present results of an H-alpha survey in the rich cluster A1689 at z=0.18, using the LDSS++ spectrograph on the AAT. We obtained spectra covering redshifted H-alpha for 522 galaxies...
Lewis, Ian, Balogh, Michael, De Propris, Roberto, Couch, Warrick, Bower, Richard, Offer, Alison, ...
We have measured the equivalent width of the H-alpha emission line for 11006 galaxies brighter than M_b=-19 (LCDM) at 0.05
Sloan Digital Sky Survey: Early data release (2002)
Stoughton, Chirs, Lupton, Rpbert H., Bernardi, Mariangela, Blanton, Michael R., Burles, Scott, Castander, Francsico J., ...
The Sloan Digital Sky Survey (SDSS) is an imaging and spectroscopic survey that will eventually cover approximately one-quarter of the celestial sphere and collect spectra of 10 6 galaxies, 100,000...
Sloan Digital Sky Survey: Early Data Release (2002)
Stoughton, Chris, Lupton, Robert H., Bernardi, Mariangela, Blanton, Michael R., Burles, Scott, Castander, Francisco J., ...
Newberg, Heidi Jo, Yanny, Brian, Rockosi, Connie, Grebel, Eva K., Rix, Hans-Walter, Brinkmann, Jon, ...
Baldry, Ivan K., Glazebrook, Karl, Bland-Hawthorn, Joss, Bridges, Terry, Cannon, Russell, Colless, Matthew, ...
not available
Baldry, Ivan K., Glazebrook, Karl, Bland-Hawthorn, Joss, Bridges, Terry, Cannon, Russell, Colless, Matthew, ...
not available
Baldry, Ivan K., Glazebrook, Karl, Bland-Hawthorn, Joss, Bridges, Terry, Cannon, Russell, Colless, Matthew, ...
not available
Baldry, Ivan K., Glazebrook, Karl, Baugh, Carlton, Bland-Hawthorn, Joss, Bridges, Terry J., Cannon, Russell D., ...
We present the first results on the history of star formation in the universe based on the "cosmic spectrum," in particular the volume-averaged, luminosity-weighted, stellar absorption-line...
Norberg, Peder, Baugh, Carlton, Hawkins, Edward, Maddox, Stephen J., Madgwick, Darren, Lahav, Ofer, ...
We investigate the dependence of galaxy clustering on luminosity and spectral type using the 2dF Galaxy Redshift Survey (2dFGRS). Spectral types are assigned using the principal-component analysis of...
The 2dF Galaxy Redshift Survey: galaxy luminosity functions per spectral type (2002)
Madgwick, Darren, Lahav, Ofer, Baldry, Ivan K., Baugh, Carlton, Bland-Hawthorn, Joss, Bridges, Terry J., ...
We calculate the optical bJ luminosity function (LF) of the 2dF Galaxy Redshift Survey (2dFGRS) for different subsets defined by their spectral properties. These spectrally selected subsets are...
The 2dF Galaxy Redshift Survey: the population of nearby radio galaxies at the 1-mJy level (2002)
Magliocchetti, Manuela, Maddox, Stephen J., Jackson, C. A., Bland-Hawthorn, Joss, Bridges, Terry J., Cannon, Russell D., ...
We use redshift determinations and spectral analysis of galaxies in the 2dF Galaxy Redshift Survey to study the properties of local radio sources with S ≥ 1 mJy. 557 objects (hereafter called the...
Sadler, Elaine M., Jackson, C. A., Cannon, Russell D., McIntyre, Vincent J., Murphy, Tara, Bland-Hawthorn, Joss, ...
We have cross-matched the 1.4-GHz NRAO VLA Sky Survey (NVSS) with the first 210 fields observed in the 2dF Galaxy Redshift Survey (2dFGRS), covering an effective area of 325 deg2 (about 20 per cent...
Lewis, Ian, Balogh, Michael L., De Propris, Roberto, Couch, Warrick J., Bower, Richard G., Offer, Alison R., ...
We have measured the equivalent width of the Ha emission line for 11 006 galaxies brighter than Mb, = -19 (ΩΛ = 0.7, Ωm = 0.3, H0 = 70 km s-1 Mpc-1) at 0.05 < z < 0.1 in the 2dF Galaxy Redshift...
The 2dF Galaxy Redshift Survey: a targeted study of catalogued clusters of galaxies (2002)
De Propris, Roberto, Couch, Warrick J., Colless, Matthew, Dalton, Gavin B., Collins, Chris A., Baugh, Carlton, ...
We have carried out a study of known clusters within the 2dF Galaxy Redshift Survey (2dFGRS) observed areas and have identified 431 Abell, 173 APM and 343 EDCC clusters. Precise redshifts, velocity...
The 2dF Galaxy Redshift Survey: the bias of galaxies and the density of the Universe (2002)
Verde, Licia, Heavens, Alan F., Percival, Will J., Matarrese, Sabino, Baugh, Carlton, Bland-Hawthorn, Joss, ...
We compute the bispectrum of the 2dF Galaxy Redshift Survey (2dFGRS) and use it to measure the bias parameter of the galaxies. This parameter quantifies the strength of clustering of the galaxies...
Sloan Digital Sky Survey: early data release (2002)
Stoughton, Chris, Lupton, Robert H., Bernardi, Mariangela, Blanton, Michael R., Burles, Scott M., Castander, Francisco J., ...
The Sloan Digital Sky Survey (SDSS) is an imaging and spectroscopic survey that will eventually cover approximately one-quarter of the celestial sphere and collect spectra of ≈ 106 galaxies,...
Percival, Will J., Sutherland, William J., Peacock, John A., Baugh, Carlton, Bland-Hawthorn, Joss, Bridges, Terry J., ...
We constrain flat cosmological models with a joint likelihood analysis of a new compilation of data from the cosmic microwave background (CMB) and from the 2dF Galaxy Redshift Survey (2dFGRS)....
Lahav, Ofer, Bridle, Sarah, Percival, Will J., Peacock, John A., Efstathiou, George P., Baugh, Carlton, ...
We compare the amplitudes of fluctuations probed by the 2dF Galaxy Redshift Survey (2dFGRS) and by the latest measurements of the cosmic microwave background (CMB) anisotropies. By combining the...
New upper limit on the total neutrino mass from the 2 Degree Field Galaxy Redshift Survey (2002)
Elgaroy, O., Lahav, Ofer, Percival, Will J., Peacock, John A., Madgwick, Darren, Bridle, Sarah, ...
We constrain fν≡Ων/Ωm, the fractional contribution of neutrinos to the total mass density in the Universe, by comparing the power spectrum of fluctuations derived from the 2 Degree Field Galaxy...
The Anglo-Australian observatory 2dF facility (2002)
Lewis, Ian J., Cannon, Russell D., Taylor, Keith, Glazebrook, Karl, Bailey, J. A., Baldry, Ivan K., ...
The 2dF (Two-degree Field) facility at the prime focus of the Anglo-Australian Telescope provides multiple-object spectroscopy over a 2° field of view. Up to 400 target fibres can be...
Efstathiou, George P., Moody, Stephen J., Peacock, John A., Percival, Will J., Baugh, Carlton, Bland-Hawthorn, Joss, ...
We perform a joint likelihood analysis of the power spectra of the 2dF Galaxy Redshift Survey (2dFGRS) and the cosmic microwave background (CMB) anisotropies under the assumptions that the initial...
Norberg, Peder, Cole, Shaun, Baugh, Carlton, Frenk, Carlos S., Baldry, Ivan K., Bland-Hawthorn, Joss, ...
We use more than 110 500 galaxies from the 2dF Galaxy Redshift Survey (2dFGRS) to estimate the bJ-band galaxy luminosity function at redshift z = 0, taking account of evolution, the distribution of...
An H alpha survey of the rich cluster A 1689 (2002)
Balogh, Michael L., Couch, Warrick J., Smail, Ian R., Bower, Richard G., Glazebrook, Karl
We present results of an Hα survey in the rich cluster A 1689 at z = 0.18, using the LDSS++ spectrograph on the Anglo-Australian Telescope (AAT). We obtained spectra covering redshifted...
Baldry, Ivan K., Glazebrook, Karl, Baugh, Carlton, Bland-Hawthorn, Joss, Bridges, Terry J., Cannon, Russell D., ...
We present the first results on the history of star formation in the universe based on the "cosmic spectrum," in particular the volume-averaged, luminosity-weighted, stellar absorption-line...
Norberg, Peder, Baugh, Carlton, Hawkins, Edward, Maddox, Stephen J., Madgwick, Darren, Lahav, Ofer, ...
We investigate the dependence of galaxy clustering on luminosity and spectral type using the 2dF Galaxy Redshift Survey (2dFGRS). Spectral types are assigned using the principal-component analysis of...
The 2dF Galaxy Redshift Survey: galaxy luminosity functions per spectral type (2002)
Madgwick, Darren, Lahav, Ofer, Baldry, Ivan K., Baugh, Carlton, Bland-Hawthorn, Joss, Bridges, Terry J., ...
We calculate the optical bJ luminosity function (LF) of the 2dF Galaxy Redshift Survey (2dFGRS) for different subsets defined by their spectral properties. These spectrally selected subsets are...
The 2dF Galaxy Redshift Survey: the population of nearby radio galaxies at the 1-mJy level (2002)
Magliocchetti, Manuela, Maddox, Stephen J., Jackson, C. A., Bland-Hawthorn, Joss, Bridges, Terry J., Cannon, Russell D., ...
We use redshift determinations and spectral analysis of galaxies in the 2dF Galaxy Redshift Survey to study the properties of local radio sources with S ≥ 1 mJy. 557 objects (hereafter called the...
Sadler, Elaine M., Jackson, C. A., Cannon, Russell D., McIntyre, Vincent J., Murphy, Tara, Bland-Hawthorn, Joss, ...
We have cross-matched the 1.4-GHz NRAO VLA Sky Survey (NVSS) with the first 210 fields observed in the 2dF Galaxy Redshift Survey (2dFGRS), covering an effective area of 325 deg2 (about 20 per cent...
Lewis, Ian, Balogh, Michael L., De Propris, Roberto, Couch, Warrick J., Bower, Richard G., Offer, Alison R., ...
We have measured the equivalent width of the Ha emission line for 11 006 galaxies brighter than Mb, = -19 (ΩΛ = 0.7, Ωm = 0.3, H0 = 70 km s-1 Mpc-1) at 0.05 < z < 0.1 in the 2dF Galaxy Redshift...
The 2dF Galaxy Redshift Survey: a targeted study of catalogued clusters of galaxies (2002)
De Propris, Roberto, Couch, Warrick J., Colless, Matthew, Dalton, Gavin B., Collins, Chris A., Baugh, Carlton, ...
We have carried out a study of known clusters within the 2dF Galaxy Redshift Survey (2dFGRS) observed areas and have identified 431 Abell, 173 APM and 343 EDCC clusters. Precise redshifts, velocity...
The 2dF Galaxy Redshift Survey: the bias of galaxies and the density of the Universe (2002)
Verde, Licia, Heavens, Alan F., Percival, Will J., Matarrese, Sabino, Baugh, Carlton, Bland-Hawthorn, Joss, ...
We compute the bispectrum of the 2dF Galaxy Redshift Survey (2dFGRS) and use it to measure the bias parameter of the galaxies. This parameter quantifies the strength of clustering of the galaxies...
Sloan Digital Sky Survey: early data release (2002)
Stoughton, Chris, Lupton, Robert H., Bernardi, Mariangela, Blanton, Michael R., Burles, Scott M., Castander, Francisco J., ...
The Sloan Digital Sky Survey (SDSS) is an imaging and spectroscopic survey that will eventually cover approximately one-quarter of the celestial sphere and collect spectra of ≈ 106 galaxies,...
Percival, Will J., Sutherland, William J., Peacock, John A., Baugh, Carlton, Bland-Hawthorn, Joss, Bridges, Terry J., ...
We constrain flat cosmological models with a joint likelihood analysis of a new compilation of data from the cosmic microwave background (CMB) and from the 2dF Galaxy Redshift Survey (2dFGRS)....
Lahav, Ofer, Bridle, Sarah, Percival, Will J., Peacock, John A., Efstathiou, George P., Baugh, Carlton, ...
We compare the amplitudes of fluctuations probed by the 2dF Galaxy Redshift Survey (2dFGRS) and by the latest measurements of the cosmic microwave background (CMB) anisotropies. By combining the...
New upper limit on the total neutrino mass from the 2 Degree Field Galaxy Redshift Survey (2002)
Elgaroy, O., Lahav, Ofer, Percival, Will J., Peacock, John A., Madgwick, Darren, Bridle, Sarah, ...
We constrain fν≡Ων/Ωm, the fractional contribution of neutrinos to the total mass density in the Universe, by comparing the power spectrum of fluctuations derived from the 2 Degree Field Galaxy...
The Anglo-Australian observatory 2dF facility (2002)
Lewis, Ian J., Cannon, Russell D., Taylor, Keith, Glazebrook, Karl, Bailey, J. A., Baldry, Ivan K., ...
The 2dF (Two-degree Field) facility at the prime focus of the Anglo-Australian Telescope provides multiple-object spectroscopy over a 2° field of view. Up to 400 target fibres can be...
Efstathiou, George P., Moody, Stephen J., Peacock, John A., Percival, Will J., Baugh, Carlton, Bland-Hawthorn, Joss, ...
We perform a joint likelihood analysis of the power spectra of the 2dF Galaxy Redshift Survey (2dFGRS) and the cosmic microwave background (CMB) anisotropies under the assumptions that the initial...
Norberg, Peder, Cole, Shaun, Baugh, Carlton, Frenk, Carlos S., Baldry, Ivan K., Bland-Hawthorn, Joss, ...
We use more than 110 500 galaxies from the 2dF Galaxy Redshift Survey (2dFGRS) to estimate the bJ-band galaxy luminosity function at redshift z = 0, taking account of evolution, the distribution of...
An H alpha survey of the rich cluster A 1689 (2002)
Balogh, Michael L., Couch, Warrick J., Smail, Ian R., Bower, Richard G., Glazebrook, Karl
We present results of an Hα survey in the rich cluster A 1689 at z = 0.18, using the LDSS++ spectrograph on the Anglo-Australian Telescope (AAT). We obtained spectra covering redshifted Hα at z =...
Baldry, Ivan K., Glazebrook, Karl, Bland-Hawthorn, Joss, Bridges, Terry, Cannon, Russell, Colless, Matthew, ...
not available
Lahav, Ofer, Bridle, Sarah L., Percival, Will J., Peacock, John A., Efstathiou, George, Baugh, Carlton M., ...
We compare the amplitudes of fluctuations probed by the 2dF Galaxy Redshift Survey and by the latest measurements of the Cosmic Microwave Background anisotropies. By combining the 2dFGRS and CMB data...
Efstathiou, George, Moody, Stephen, Peacock, John A., Percival, Will J., Baugh, Carlton, Bland-Hawthorn, Joss, ...
We perform a joint likelihood analysis of the power spectra of the 2dF Galaxy Redshift Survey (2dFGRS) and the cosmic microwave background (CMB) anisotropies under the assumptions that the initial...
The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe (2001)
Percival, Will J., Baugh, Carlton M., Bland-Hawthorn, Joss, Bridges, Terry, Cannon, Russell, Cole, Shaun, ...
The 2dF Galaxy Redshift Survey has now measured in excess of 160000 galaxy redshifts. This paper presents the power spectrum of the galaxy distribution, calculated using a direct FFT-based technique....
The 2dF galaxy redshift survey: near-infrared galaxy luminosity functions (2001)
Cole, Shaun, Norberg, Peder, Baugh, Carlton, Frenk, Carlos S., Bland-Hawthorn, Joss, Bridges, Terry J., ...
We combine the Two Micron All Sky Survey (2MASS) Extended Source Catalogue and the 2dF Galaxy Redshift Survey to produce an infrared selected galaxy catalogue with 17 173 measured redshifts. We use...
Microslit nod-shuffle spectroscopy: a technique for achieving very high densities of spectra (2001)
Glazebrook, Karl, Bland-Hawthorn, Joss
We describe a new approach to obtaining very high surface densities of optical spectra in astronomical observations with extremely accurate subtraction of night sky emission. The observing technique...
The 2dF Galaxy Redshift Survey: luminosity dependence of galaxy clustering (2001)
Norberg, Peder, Baugh, Carlton, Hawkins, Edward, Maddox, Stephen J., Peacock, John A., Cole, Shaun, ...
We investigate the dependence of the strength of galaxy clustering on intrinsic luminosity using the Anglo-Australian two degree field galaxy redshift survey (2dFGRS). The 2dFGRS is over an order of...
The 2dF Galaxy Redshift Survey: spectra and redshifts (2001)
Colless, Matthew, Dalton, Gavin B., Maddox, Stephen J., Sutherland, William J., Norberg, Peder, Cole, Shaun, ...
The 2dF Galaxy Redshift Survey (2dFGRS) is designed to measure redshifts for approximately 250 000 galaxies. This paper describes the survey design, the spectroscopic observations, the redshift...
The 2dF Galaxy Redshift Survey: the power spectrum and the matter content of the Universe (2001)
Percival, Will J., Baugh, Carlton, Bland-Hawthorn, Joss, Bridges, Terry J., Cannon, Russell D., Cole, Shaun, ...
The 2dF Galaxy Redshift Survey has now measured in excess of 160 000 galaxy redshifts. This paper presents the power spectrum of the galaxy distribution, calculated using a direct Fourier transform...
A low global star formation rate in the rich galaxy cluster AC 114 at z=0.32 (2001)
Couch, Warrick J., Balogh, Michael L., Bower, Richard G., Smail, Ian R., Glazebrook, Karl, Taylor, Melinda
We present the results of a wide-field survey for Hα-emitting galaxies in the cluster AC 114 at z = 0.32. Spectra centered on Hα at the cluster redshift have been obtained for 586 galaxies to Itot...
The 2dF Galaxy Redshift Survey: the number and luminosity density of galaxies (2001)
Cross, Nicholas J. G., Driver, Simon P., Couch, Warrick, Baugh, Carlton, Bland-Hawthorn, Joss, Bridges, Terry J., ...
We present the bivariate brightness distribution (BBD) for the 2dF Galaxy Redshift Survey (2dFGRS) based on a preliminary subsample of 45 000 galaxies. The BBD is an extension of the galaxy...
The 2dF Galaxy Redshift Survey: near-infrared galaxy luminosity functions (2001)
Cole, Shaun, Norberg, Peder, Baugh, Carlton, Frenk, Carlos S., Bland-Hawthorn, Joss, Bridges, Terry J., ...
We combine the Two Micron All Sky Survey (2MASS) Extended Source Catalogue and the 2dF Galaxy Redshift Survey to produce an infrared selected galaxy catalogue with 17 173 measured redshifts. We use...
Microslit nod-shuffle spectroscopy: a technique for achieving very high densities of spectra (2001)
Glazebrook, Karl, Bland-Hawthorn, Joss
We describe a new approach to obtaining very high surface densities of optical spectra in astronomical observations with extremely accurate subtraction of night sky emission. The observing technique...
The 2dF Galaxy Redshift Survey: luminosity dependence of galaxy clustering (2001)
Norberg, Peder, Baugh, Carlton, Hawkins, Edward, Maddox, Stephen J., Peacock, John A., Cole, Shaun, ...
We investigate the dependence of the strength of galaxy clustering on intrinsic luminosity using the Anglo-Australian two degree field galaxy redshift survey (2dFGRS). The 2dFGRS is over an order of...
The 2dF Galaxy Redshift Survey: spectra and redshifts (2001)
Colless, Matthew, Dalton, Gavin B., Maddox, Stephen J., Sutherland, William J., Norberg, Peder, Cole, Shaun, ...
The 2dF Galaxy Redshift Survey (2dFGRS) is designed to measure redshifts for approximately 250 000 galaxies. This paper describes the survey design, the spectroscopic observations, the redshift...
The 2dF Galaxy Redshift Survey: the power spectrum and the matter content of the Universe (2001)
Percival, Will J., Baugh, Carlton, Bland-Hawthorn, Joss, Bridges, Terry J., Cannon, Russell D., Cole, Shaun, ...
The 2dF Galaxy Redshift Survey has now measured in excess of 160 000 galaxy redshifts. This paper presents the power spectrum of the galaxy distribution, calculated using a direct Fourier transform...
A low global star formation rate in the rich galaxy cluster AC 114 at z=0.32 (2001)
Couch, Warrick J., Balogh, Michael L., Bower, Richard G., Smail, Ian R., Glazebrook, Karl, Taylor, Melinda
We present the results of a wide-field survey for Hα-emitting galaxies in the cluster AC 114 at z = 0.32. Spectra centered on Hα at the cluster redshift have been obtained for 586 galaxies to Itot...
The 2dF Galaxy Redshift Survey: the number and luminosity density of galaxies (2001)
Cross, Nicholas J. G., Driver, Simon P., Couch, Warrick, Baugh, Carlton, Bland-Hawthorn, Joss, Bridges, Terry J., ...
We present the bivariate brightness distribution (BBD) for the 2dF Galaxy Redshift Survey (2dFGRS) based on a preliminary subsample of 45 000 galaxies. The BBD is an extension of the galaxy...
Peacock, John A., Cole, Shaun, Norberg, Peder, Baugh, Carlton M., Bland-Hawthorn, Joss, Bridges, Terry, ...
The large-scale structure in the distribution of galaxies is thought to arise from the gravitational instability of small fluctuations in the initial density field of the Universe. A key test of this...
The 2dF Galaxy Redshift Survey: Near Infrared Galaxy Luminosity Functions (2000)
Cole, Shaun, Norberg, Peder, Baugh, Carlton, Frenk, Carlos, Bland-Hawthorn, Joss, Bridges, Terry, ...
We combine the 2MASS extended source catalogue and the 2dFGRS to produce an IR selected galaxy catalogue with 17,173 measured redshifts. We use this extensive dataset to estimate the J and K-band...
The 2dF Galaxy Redshift Survey: The Number and Luminosity Density of Galaxies (2000)
Cross, Nicholas, Driver, Simon P., Couch, Warrick, Baugh, Carlton M., Bland-Hawthorn, Joss, Bridges, Terry, ...
We present the bivariate brightness distribution (BBD) for the 2dF Galaxy Redshift Survey (2dFGRS) based on a preliminary subsample of 45,000 galaxies. The BBD is an extension of the galaxy...
Microslit Nod-shuffle Spectroscopy - a technique for achieving very high densities of spectra (2000)
Glazebrook, Karl, Bland-Hawthorn, Joss
We describe a new approach to obtaining very high surface densities of optical spectra in astronomical observations with extremely accurate subtraction of night sky emission. The observing technique...
A low global star formation rate in the rich galaxy cluster AC114 at z=0.32 (2000)
Couch, Warrick J., Balogh, Michael L., Bower, Richard G., Smail, Ian, Glazebrook, Karl, Taylor, Melinda
We present the results of a wide-field survey for H-alpha emitting galaxies in the cluster AC114 at z=0.32. Spectra centred on H-alpha at the cluster redshift have been obtained for 586 galaxies to...
Le Fevre, Olivier, Abraham, Roberto G., Lilly, Simon J., Ellis, Richard S., Brinchmann, Jarle, Schade, David J., ...
Hubble Space Telescope images of a sample of 285 galaxies with measured redshifts from the Canada-France Redshift Survey (CFRS) and Autofib-Low Dispersion Spectrograph Survey (LDSS) redshift surveys...
Discovery of the optical counterpart and early optical observations of GRB 990712 (2000)
Sahu, Kailash C., Vreeswijk, P. M., Bakos, Gaspar A., Menzies, John W., Bragaglia, Angela, Frontera, Filippo, ...
We present the discovery observations of the optical counterpart of the gamma-ray burst GRB 990712 taken 4.16 hr after the outburst and discuss its light curve observed in the V, R, and I bands...
Le Fevre, Olivier, Abraham, Roberto G., Lilly, Simon J., Ellis, Richard S., Brinchmann, Jarle, Schade, David J., ...
Hubble Space Telescope images of a sample of 285 galaxies with measured redshifts from the Canada-France Redshift Survey (CFRS) and Autofib-Low Dispersion Spectrograph Survey (LDSS) redshift surveys...
Discovery of the optical counterpart and early optical observations of GRB 990712 (2000)
Sahu, Kailash C., Vreeswijk, P. M., Bakos, Gaspar A., Menzies, John W., Bragaglia, Angela, Frontera, Filippo, ...
We present the discovery observations of the optical counterpart of the gamma-ray burst GRB 990712 taken 4.16 hr after the outburst and discuss its light curve observed in the V, R, and I bands...
Measurement of the star formation rate from Halpha in field galaxies at z=1 (1999)
Glazebrook, Karl, Blake, Chris, Economou, Frossie, Lilly, Simon, Colless, Matthew
We report the results of J-band infrared spectroscopy of a sample of 13 z=1 field galaxies drawn from the Canada-France Redshift Survey, targeting galaxies with redshifts that place the rest-frame...
Measurement of the star formation rate from Halpha in field galaxies at z=1 (1999)
Glazebrook, Karl, Blake, Chris, Economou, Frossie, Lilly, Simon, Colless, Matthew
We report the results of J-band infrared spectroscopy of a sample of 13 z=1 field galaxies drawn from the Canada-France Redshift Survey, targeting galaxies with redshifts that place the rest-frame...
Emission line galaxies at 1 less than z less than 1.5 (1999)
Glazebrook, Karl, Abraham, R. G., Blake, C. A.
Abstract not available.
The 2dF Galaxy Redshift Survey: spectral types and luminosity functions (1999)
Folkes, Simon, Ronen, Shai, Price, Ian, Lahav, Ofer, Colless, Matthew, Maddox, Stephen J., ...
We describe the 2dF Galaxy Redshift Survey (2dFGRS) and the current status of the observations. In this exploratory paper, we apply a principal component analysis to a preliminary sample of 5869...
Abraham, Roberto G., Ellis, Richard S., Fabian, Andrew C., Tanvir, Nial R., Glazebrook, Karl
We analyse the spatially resolved colours of distant galaxies of known redshift in the Hubble Deep Field, using a new technique based on matching resolved four-band colour data to the predictions of...
Measurement of the star formation rate from H alpha in field galaxies at z=1 (1999)
Glazebrook, Karl, Blake, Chris, Economou, Frossie, Lilly, Simon J., Colless, Matthew
We report the results of J-band infrared spectroscopy of a sample of 13 z = 1 field galaxies drawn from the Canada-France Redshift Survey, targeting galaxies with redshifts that place the rest-frame...
Schade, David J., Lilly, Simon J., Crampton, David, Ellis, Richard S., Le Fevre, Olivier, Hammer, Francois, ...
Two-dimensional surface photometry has been performed on a magnitude-limited sample of 46 field galaxies that are classified as ellipticals based on two-dimensional fitting of their luminosity...
Emission line galaxies at 1 less than z less than 1.5 (1999)
Glazebrook, Karl, Abraham, R. G., Blake, C. A.
Abstract not available.
The 2dF Galaxy Redshift Survey: spectral types and luminosity functions (1999)
Folkes, Simon, Ronen, Shai, Price, Ian, Lahav, Ofer, Colless, Matthew, Maddox, Stephen J., ...
We describe the 2dF Galaxy Redshift Survey (2dFGRS) and the current status of the observations. In this exploratory paper, we apply a principal component analysis to a preliminary sample of 5869...
Abraham, Roberto G., Ellis, Richard S., Fabian, Andrew C., Tanvir, Nial R., Glazebrook, Karl
We analyse the spatially resolved colours of distant galaxies of known redshift in the Hubble Deep Field, using a new technique based on matching resolved four-band colour data to the predictions of...
Measurement of the star formation rate from H alpha in field galaxies at z=1 (1999)
Glazebrook, Karl, Blake, Chris, Economou, Frossie, Lilly, Simon J., Colless, Matthew
We report the results of J-band infrared spectroscopy of a sample of 13 z = 1 field galaxies drawn from the Canada-France Redshift Survey, targeting galaxies with redshifts that place the rest-frame...
Schade, David J., Lilly, Simon J., Crampton, David, Ellis, Richard S., Le Fevre, Olivier, Hammer, Francois, ...
Two-dimensional surface photometry has been performed on a magnitude-limited sample of 46 field galaxies that are classified as ellipticals based on two-dimensional fitting of their luminosity...
Measurement of the star formation rate from Halpha in field galaxies at z=1 (1999)
Glazebrook, Karl, Blake, Chris, Economou, Frossie, Lilly, Simon, Colless, Matthew
We report the results of J-band infrared spectroscopy of a sample of 13 z=1 field galaxies drawn from the Canada-France Redshift Survey, targeting galaxies with redshifts that place the rest-frame...
Measurement of Star-Formation Rate from H-alpha in field galaxies at z=1 (1998)
Glazebrook, Karl, Blake, Chris, Economou, Frossie, Lilly, Simon, Colless, Matthew
We report the results of J-band infrared spectroscopy of a sample of 13 z=1 field galaxies drawn from the Canada-France Redshift Survey, targeting galaxies whose redshifts place the rest frame...
Lilly, Simon, Schade, David, Ellis, Richard, Le Fevre, Oliver, Brinchmann, Jarle, Tresse, Laurence, ...
Several aspects of the evolution of star-forming galaxies are studied using measures of the two-dimensional surface brightness profiles extracted from Hubble Space Telescope images of a sample of 341...
Brinchmann, Jarle, Abraham, Roberto, Schade, David, Tresse, Laurence, Ellis, Richard S., Lilly, Simon, ...
We analyze Hubble Space Telescope images of a complete sample of 341 galaxies drawn from the CFRS and LDSS ground-based redshift surveys. In this, the first paper in the series, each galaxy has been...
Brinchmann, Jarle, Abraham, Roberto, Schade, David, Tresse, Laurence, Ellis, Richard S., Lilly, Simon, ...
We analyze Hubble Space Telescope images of a complete sample of 341 galaxies drawn from the CFRS and LDSS ground-based redshift surveys. In this, the first paper in the series, each galaxy has been...
Lilly, Simon, Schade, David, Ellis, Richard, Le Fevre, Oliver, Brinchmann, Jarle, Tresse, Laurence, ...
Several aspects of the evolution of star-forming galaxies are studied using measures of the two-dimensional surface brightness profiles extracted from Hubble Space Telescope images of a sample of 341...
Brinchmann, Jarle, Abraham, Roberto, Schade, David, Tresse, Laurence, Ellis, Richard S., Lilly, Simon, ...
We analyze Hubble Space Telescope images of a complete sample of 341 galaxies drawn from the CFRS and LDSS ground-based redshift surveys. In this, the first paper in the series, each galaxy has been...
Lilly, Simon, Schade, David, Ellis, Richard, Le Fevre, Oliver, Brinchmann, Jarle, Tresse, Laurence, ...
Several aspects of the evolution of star-forming galaxies are studied using measures of the two-dimensional surface brightness profiles extracted from Hubble Space Telescope images of a sample of 341...
Brinchmann, Jarle, Abraham, Roberto G., Schade, David J., Tresse, Laurence, Ellis, Richard S., Lilly, Simon J., ...
We analyze Hubble Space Telescope images of a complete sample of 341 galaxies drawn from the CFRS and LDSS ground-based redshift surveys. In this, the first paper in the series, each galaxy has been...
Tyson, J. Anthony, Fischer, Philippe, Guhathakurta, Puragra, McIlroy, Peter, Wenk, R. A., Huchra, John P., ...
Deep Hubble Space Telescope Wide Field Camera (WFC-1) imaging of a region 3farcm7 east of the V = 13 mag Seyfert galaxy NGC 5548 in the F555W and F785LP bands, and deep ground-based V and I imaging,...
Lilly, Simon J., Schade, David J., Ellis, Richard S., Le Fevre, Olivier, Brinchmann, Jarle, Tresse, Laurence, ...
Several aspects of the evolution of star-forming galaxies are studied using measures of the two-dimensional surface brightness profiles extracted from Hubble Space Telescope images of a sample of 341...
The physical parameters of the evolving population of faint galaxies (1998)
Glazebrook, Karl, Abraham, Roberto G., Santiago, Basilio X., Ellis, Richard S., Griffiths, Richard E.
The excess number of blue galaxies at faint magnitudes is a subject of much controversy. Recent Hubble Space Telescope results have revealed a plethora of galaxies with peculiar morphologies...
Brinchmann, Jarle, Abraham, Roberto G., Schade, David J., Tresse, Laurence, Ellis, Richard S., Lilly, Simon J., ...
We analyze Hubble Space Telescope images of a complete sample of 341 galaxies drawn from the CFRS and LDSS ground-based redshift surveys. In this, the first paper in the series, each galaxy has been...
Tyson, J. Anthony, Fischer, Philippe, Guhathakurta, Puragra, McIlroy, Peter, Wenk, R. A., Huchra, John P., ...
Deep Hubble Space Telescope Wide Field Camera (WFC-1) imaging of a region 3farcm7 east of the V = 13 mag Seyfert galaxy NGC 5548 in the F555W and F785LP bands, and deep ground-based V and I imaging,...
Lilly, Simon J., Schade, David J., Ellis, Richard S., Le Fevre, Olivier, Brinchmann, Jarle, Tresse, Laurence, ...
Several aspects of the evolution of star-forming galaxies are studied using measures of the two-dimensional surface brightness profiles extracted from Hubble Space Telescope images of a sample of 341...
The physical parameters of the evolving population of faint galaxies (1998)
Glazebrook, Karl, Abraham, Roberto G., Santiago, Basilio X., Ellis, Richard S., Griffiths, Richard E.
The excess number of blue galaxies at faint magnitudes is a subject of much controversy. Recent Hubble Space Telescope results have revealed a plethora of galaxies with peculiar morphologies...
Brinchmann, Jarle, Abraham, Roberto, Schade, David, Tresse, Laurence, Ellis, Richard S., Lilly, Simon, ...
We analyze Hubble Space Telescope images of a complete sample of 341 galaxies drawn from the CFRS and LDSS ground-based redshift surveys. In this, the first paper in the series, each galaxy has been...
Lilly, Simon, Schade, David, Ellis, Richard, Le Fevre, Oliver, Brinchmann, Jarle, Tresse, Laurence, ...
Several aspects of the evolution of star-forming galaxies are studied using measures of the two-dimensional surface brightness profiles extracted from Hubble Space Telescope images of a sample of 341...
The physical parameters of the evolving population of faint galaxies (1997)
Glazebrook, Karl, Abraham, Roberto, Santiago, Basilio, Ellis, Richard, Griffiths, Richard
The excess numbers of blue galaxies at faint magnitudes is a subject of much controversy. Recent Hubble Space Telescope results has revealed a plethora of galaxies with peculiar morphologies...
Automatic Redshift Determination by use of Principal Component Analysis --- I: Fundamentals (1997)
Glazebrook, Karl, Offer, Alison R., Deeley, Kathryn
With the advent of very large redshift surveys of tens to hundreds of thousands of galaxies reliable techniques for automatically determining galaxy redshifts are becoming increasingly important. The...
Perlmutter, Saul, Gabi, S., Goldhaber, G., Goobar, Ariel, Groom, Donald E., Hook, Isobel, ...
We have developed a technique to systematically discover and study high-redshift supernovae that can be used to measure the cosmological parameters. We report here results based on the initial seven...
The HST Medium Deep Survey: progress towards resolution of the faint blue galaxy problem (1997)
Griffiths, Richard, Ratnatunga, Kavan U., Casertano, Stefano, Im, Myungshin, Neuschaefer, Lyman W., Ostrander, Eric J., ...
WFPC2 on HST has provided the means to make rapid progress towards solving a long-standing problem in observational cosmology, viz. the nature of the objects contributing to the faint blue galaxy...
Optical/near-infrared observations of GRO J1744-28 (1997)
Cole, David M., Van Den Berk, Daniel E., Severson, Scott A., Miller, M. Coleman, Quashnock, J. M., Nichol, Robert C., ...
We present results from a series of optical (g- and r-band) and near-infrared (K'-band) observations of the region of the sky including the entire Rossi X-Ray Tinting Explorer and ROSAT error circles...
Kim, Alex G., Gabi, S., Goldhaber, G., Groom, Donald E., Hook, Isobel, Kim, Min Kook, ...
The Supernova Cosmology Project has discovered over 28 supernovae (SNs) at 0.35 < z < 0.65 in an ongoing program that uses Type Ia SNs (SN Ia's) as high-redshift distance indicators. Here we...
Perlmutter, Saul, Gabi, S., Goldhaber, G., Goobar, Ariel, Groom, Donald E., Hook, Isobel, ...
We have developed a technique to systematically discover and study high-redshift supernovae that can be used to measure the cosmological parameters. We report here results based on the initial seven...
The HST Medium Deep Survey: progress towards resolution of the faint blue galaxy problem (1997)
Griffiths, Richard, Ratnatunga, Kavan U., Casertano, Stefano, Im, Myungshin, Neuschaefer, Lyman W., Ostrander, Eric J., ...
WFPC2 on HST has provided the means to make rapid progress towards solving a long-standing problem in observational cosmology, viz. the nature of the objects contributing to the faint blue galaxy...
Optical/near-infrared observations of GRO J1744-28 (1997)
Cole, David M., Van Den Berk, Daniel E., Severson, Scott A., Miller, M. Coleman, Quashnock, J. M., Nichol, Robert C., ...
We present results from a series of optical (g- and r-band) and near-infrared (K'-band) observations of the region of the sky including the entire Rossi X-Ray Tinting Explorer and ROSAT error circles...
Kim, Alex G., Gabi, S., Goldhaber, G., Groom, Donald E., Hook, Isobel, Kim, Min Kook, ...
The Supernova Cosmology Project has discovered over 28 supernovae (SNs) at 0.35 < z < 0.65 in an ongoing program that uses Type Ia SNs (SN Ia's) as high-redshift distance indicators. Here we...
A Morphological Catalog of Galaxies in the Hubble Deep Field (1996)
Bergh, Sidney Van Den, Abraham, Roberto, Tanvir, Richard Ellis Nial, Santiago, Basilio, Glazebrook, Karl
We present a catalog of morphological and color data for galaxies with $I < 25$ mag in the {\em Hubble Deep Field} (Williams et al. 1996). Galaxies have been inspected and (when possible)...
Autofib Redshift Survey - I. Evolution of the galaxy luminosity function (1996)
Ellis, Richard S., Colless, Matthew, Broadhurst, Tom, Heyl, Jeremy, Glazebrook, Karl
We present a detailed determination of the rest frame B-band galaxy luminosity function (LF) as a function of redshift and star formation activity from z=0 to z~=0.75. The data set used for this...
Autofib Redshift Survey - I. Evolution of the galaxy luminosity function (1996)
Ellis, Richard S., Colless, Matthew, Broadhurst, Tom, Heyl, Jeremy, Glazebrook, Karl
We present a detailed determination of the rest frame B-band galaxy luminosity function (LF) as a function of redshift and star formation activity from z=0 to z~=0.75. The data set used for this...
The HST Medium Deep Survey: galaxy morphology at high redshift (1996)
Griffiths, R., Ratnatunga, K. U., Casertano, S., Im, M., Neuschaefer, L. W., Ellis, R., ...
With HST and WFPC2, galaxies in the Medium Deep Survey can be reliably classified to magnitudes I-814 less than or similar to 22.0 in the F814W band, at a mean redshift (z) over bar similar to 0.5....
Abraham, Roberto G., Van Den Bergh, Sidney D., Glazebrook, Karl, Ellis, Richard S., Santiago, Basilio X., Surma, P., ...
The morphological properties of high-redshift galaxies are investigated using a sample of 507 objects (I < 22.0 mag) from the Hubble Space Telescope (HST) Medium Deep Survey. Independent visual...
The type Ia supernova rate at z similar to 0.4 (1996)
Pain, Reynald, Hook, Isobel, Deustua, Susana E., Gabi, S., Goldhaber, G., Groom, Donald E., ...
We present the first measurement of the rate of Type la supernovae at high redshift. The result is derived by using a large subset of data from the Supernova Cosmology Project. Three supernovae were...
Galaxy morphology to I=25 mag in the Hubble Deep Field (1996)
Abraham, Roberto G., Tanvir, Nial R., Santiago, Basilio X., Ellis, Richard S., Glazebrook, Karl, Van Den Bergh, Sidney D.
The morphological properties of galaxies in the range 21 < I < 25 mag in the Hubble Deep Field are investigated using a quantitative classification system based on measurements of the central...
Autofib redshift survey 1: evolution of the galaxy luminosity function (1996)
Ellis, Richard S., Colless, Matthew, Broadhurst, Thomas J., Heyl, Jeremy S., Glazebrook, Karl
We present a detailed determination of the rest frame B-band galaxy luminosity function (LF) as a function of redshift and star formation activity from z = 0 to 2 ≃ 0.75. The data set used for...
A morphological catalog of galaxies in the Hubble Deep Field (1996)
Van Den Bergh, Sidney D., Abraham, Roberto G., Ellis, Richard S., Tanvir, Nial R., Santiago, Basilio X., Glazebrook, Karl
We present a catalog of morphological and color data for galaxies with 21 < I814 < 25 mag in the Hubble Deep Field (Williams et al. 1996). Galaxies have been inspected and (when possible)...
Design-Led Software Strategy for the . . . (1996)
Keith Taylor, Jeremy Bailey, Tim Wilkins, Keith Shortridge, Karl Glazebrook
. We describe the novel approach used for the software developed for the 2dF survey spectrograph. 2dF is a 400-fiber multi-object spectrograph designed for the Anglo-Australian Telescope. One of its...
The HST Medium Deep Survey: galaxy morphology at high redshift (1996)
Griffiths, R., Ratnatunga, K. U., Casertano, S., Im, M., Neuschaefer, L. W., Ellis, R., ...
With HST and WFPC2, galaxies in the Medium Deep Survey can be reliably classified to magnitudes I-814 less than or similar to 22.0 in the F814W band, at a mean redshift (z) over bar similar to 0.5....
Abraham, Roberto G., Van Den Bergh, Sidney D., Glazebrook, Karl, Ellis, Richard S., Santiago, Basilio X., Surma, P., ...
The morphological properties of high-redshift galaxies are investigated using a sample of 507 objects (I < 22.0 mag) from the Hubble Space Telescope (HST) Medium Deep Survey. Independent visual...
The type Ia supernova rate at z similar to 0.4 (1996)
Pain, Reynald, Hook, Isobel, Deustua, Susana E., Gabi, S., Goldhaber, G., Groom, Donald E., ...
We present the first measurement of the rate of Type la supernovae at high redshift. The result is derived by using a large subset of data from the Supernova Cosmology Project. Three supernovae were...
Galaxy morphology to I=25 mag in the Hubble Deep Field (1996)
Abraham, Roberto G., Tanvir, Nial R., Santiago, Basilio X., Ellis, Richard S., Glazebrook, Karl, Van Den Bergh, Sidney D.
The morphological properties of galaxies in the range 21 < I < 25 mag in the Hubble Deep Field are investigated using a quantitative classification system based on measurements of the central...
Autofib redshift survey 1: evolution of the galaxy luminosity function (1996)
Ellis, Richard S., Colless, Matthew, Broadhurst, Thomas J., Heyl, Jeremy S., Glazebrook, Karl
We present a detailed determination of the rest frame B-band galaxy luminosity function (LF) as a function of redshift and star formation activity from z = 0 to 2 ≃ 0.75. The data set used for this...
A morphological catalog of galaxies in the Hubble Deep Field (1996)
Van Den Bergh, Sidney D., Abraham, Roberto G., Ellis, Richard S., Tanvir, Nial R., Santiago, Basilio X., Glazebrook, Karl
We present a catalog of morphological and color data for galaxies with 21 < I814 < 25 mag in the Hubble Deep Field (Williams et al. 1996). Galaxies have been inspected and (when possible)...
Autofib Redshift Survey - I. Evolution of the galaxy luminosity function (1996)
Ellis, Richard S., Colless, Matthew, Broadhurst, Tom, Heyl, Jeremy, Glazebrook, Karl
We present a detailed determination of the rest frame B-band galaxy luminosity function (LF) as a function of redshift and star formation activity from z=0 to z~=0.75. The data set used for this...
Autofib Redshift Survey - I. Evolution of the Galaxy Luminosity Function (1995)
Ellis, Richard S., Colless, Matthew, Broadhurst, Tom, Heyl, Jeremy, Glazebrook, Karl
We present a detailed determination of the restframe B-band galaxy luminosity function (LF) as a function of redshift and star formation activity from z=0 to z=0.75. The dataset used for this purpose...
The morphological identification of the rapidly evolving population of faint galaxies (1995)
Glazebrook, Karl, Ellis, Richard, Santiago, Basilio, Griffiths, Richard
The excess numbers of blue galaxies at faint magnitudes are a long-standing cosmological puzzle. We present new number-magnitude counts as a function of galactic morphology from the first deep fields...
AN IMAGING K-BAND SURVEY - II: THE REDSHIFT SURVEY AND GALAXY EVOLUTION IN THE INFRARED (1995)
Glazebrook, Karl, Peacock, J. A., Miller, L., Collins, C. A.
We present a redshift survey of 124 galaxies, from an imaging $K$-band survey complete to $K\simeq 17.3$. The optical-to-infrared colours are consistent with the range expected from synthetic galaxy...
A faint galaxy redshift survey to B=24 (1995)
Glazebrook, Karl, Ellis, Richard, Colless, Matthew, Broadhurst, Tom, Allington-Smith, Jeremy, Tanvir, Nial
Using the multislit LDSS-2 spectrograph on the William Herschel Telescope, we have completed a redshift survey in the magnitude range 22.5<B<24 which has produced 73 redshifts, representing a...
A faint galaxy redshift survey to B=24 (1995)
Glazebrook, Karl, Ellis, Richard, Colless, Matthew, Broadhurst, Tom, Allington-Smith, Jeremy, Tanvir, Nial
Using the multislit LDSS-2 spectrograph on the William Herschel Telescope, we have completed a redshift survey in the magnitude range 22.5
A faint galaxy redshift survey to B=24 (1995)
Glazebrook, Karl, Ellis, Richard, Colless, Matthew, Broadhurst, Tom, Allington-Smith, Jeremy, Tanvir, Nial
Using the multislit LDSS-2 spectrograph on the William Herschel Telescope, we have completed a redshift survey in the magnitude range 22.5
The morphological identification of the rapidly evolving population of faint galaxies (1995)
Glazebrook, Karl, Ellis, Richard S., Santiago, Basilio X., Griffiths, Richard
The excess numbers of blue galaxies at faint magnitudes are a long-standing cosmological puzzle. We present new number-magnitude counts as a function of galactic morphology from the first deep fields...
A faint galaxy redshift survey to B=24 (1995)
Glazebrook, Karl, Ellis, Richard S., Colless, Matthew, Broadhurst, Thomas J., Allington-Smith, Jeremy, Tanvir, Nial R.
Using the multislit LDSS-2 spectrograph on the William Herschel Telescope, we have completed a redshift survey in the magnitude range 22.5
The morphological identification of the rapidly evolving population of faint galaxies (1995)
Glazebrook, Karl, Ellis, Richard S., Santiago, Basilio X., Griffiths, Richard
The excess numbers of blue galaxies at faint magnitudes are a long-standing cosmological puzzle. We present new number-magnitude counts as a function of galactic morphology from the first deep fields...
A faint galaxy redshift survey to B=24 (1995)
Glazebrook, Karl, Ellis, Richard S., Colless, Matthew, Broadhurst, Thomas J., Allington-Smith, Jeremy, Tanvir, Nial R.
Using the multislit LDSS-2 spectrograph on the William Herschel Telescope we have completed a redshift survey in the magnitude range 22.5 < B < 24 which has produced 73 redshifts representing a 73%...
A faint galaxy redshift survey to B=24 (1995)
Glazebrook, Karl, Ellis, Richard, Colless, Matthew, Broadhurst, Tom, Allington-Smith, Jeremy, Tanvir, Nial
Using the multislit LDSS-2 spectrograph on the William Herschel Telescope, we have completed a redshift survey in the magnitude range 22.5
A low-dispersion survey spectrograph (LDSS-2) for the William Herschel Telescope (1994)
Allingtonsmith, J., Breare, M., Ellis, R., Gellatly, D., Glazebrook, Karl, Jorden, P., ...
LDSS-2 is a wide-field, multiaperture spectrograph recently installed on the 4.2-m William Herschel Telescope (WHT) in La Palma. The spectrograph has high system throughput (including the telescope...
The theta-z relation for HST bulges and disks out to z similar or equal to 0.8 (1994)
Mutz, Steven B., Windhorst, Rogier A., Schmidtke, Paul C., Pascarelle, Sebastian M., Griffiths, Richard E., Ratnatunga, Kavan U., ...
We present HST scale lengths and ground-based redshifts for 63 faint field galaxies down to 1 ≲ 21.5 mag from the Medium-Deep Survey. These have measured redshifts z ≲ 0.8 and half-light...
The morphology of faint galaxies in medium deep survey images using WFPC2 (1994)
Griffiths, Richard, Casertano, Stefano, Ratnatunga, Kavan U., Neuschaefer, Lyman W., Ellis, Richard S., Gilmore, Gerard F., ...
First results from HST Medium Deep Survey images taken with WFPC2 demonstrate that galaxy classifications can be reliably performed to magnitudes I814 less-than-or-similar-to 22.0 in the F815W band....
Windhorst, Rogier A., Schmidtke, Paul C., Pascarelle, Sebastian M., Gordon, J. M., Griffiths, Richard, Ratnatunga, Kavan U., ...
We present isophotal profiles of six faint field galaxies from some of the first deep images taken for the Hubble Space Telescope (HST) Medium Deep Survey (MDS). These have redshifts in the range...
Glazebrook, Karl, Lehar, Joseph, Ellis, Richard S., Aragon-Salamanca, Alfonso, Griffiths, Richard
We report the discovery of an object with a very peculiar structure, using observations from the refurbished Hubble Space Telescope (HST) as part of the Medium-Deep Survey project. The object...
Griffiths, Richard, Ratnatunga, Kavan U., Neuschaefer, Lyman W., Casertano, Stefano, Im, Myungshin, Wyckoff, Eric W., ...
We present results from the Medium Deep Survey (MDS), a Key Project using the Hubble Space Telescope. Wide Field Camera images of random fields have been taken in "parallel mode" with an effective...
A low-dispersion survey spectrograph (LDSS-2) for the William Herschel Telescope (1994)
Allingtonsmith, J., Breare, M., Ellis, R., Gellatly, D., Glazebrook, Karl, Jorden, P., ...
LDSS-2 is a wide-field, multiaperture spectrograph recently installed on the 4.2-m William Herschel Telescope (WHT) in La Palma. The spectrograph has high system throughput (including the telescope...
The theta-z relation for HST bulges and disks out to z similar or equal to 0.8 (1994)
Mutz, Steven B., Windhorst, Rogier A., Schmidtke, Paul C., Pascarelle, Sebastian M., Griffiths, Richard E., Ratnatunga, Kavan U., ...
We present HST scale lengths and ground-based redshifts for 63 faint field galaxies down to 1 ≲ 21.5 mag from the Medium-Deep Survey. These have measured redshifts z ≲ 0.8 and half-light...
The morphology of faint galaxies in medium deep survey images using WFPC2 (1994)
Griffiths, Richard, Casertano, Stefano, Ratnatunga, Kavan U., Neuschaefer, Lyman W., Ellis, Richard S., Gilmore, Gerard F., ...
First results from HST Medium Deep Survey images taken with WFPC2 demonstrate that galaxy classifications can be reliably performed to magnitudes I814 less-than-or-similar-to 22.0 in the F815W band....
Windhorst, Rogier A., Schmidtke, Paul C., Pascarelle, Sebastian M., Gordon, J. M., Griffiths, Richard, Ratnatunga, Kavan U., ...
We present isophotal profiles of six faint field galaxies from some of the first deep images taken for the Hubble Space Telescope (HST) Medium Deep Survey (MDS). These have redshifts in the range...
Glazebrook, Karl, Lehar, Joseph, Ellis, Richard S., Aragon-Salamanca, Alfonso, Griffiths, Richard
We report the discovery of an object with a very peculiar structure, using observations from the refurbished Hubble Space Telescope (HST) as part of the Medium-Deep Survey project. The object...
Griffiths, Richard, Ratnatunga, Kavan U., Neuschaefer, Lyman W., Casertano, Stefano, Im, Myungshin, Wyckoff, Eric W., ...
We present results from the Medium Deep Survey (MDS), a Key Project using the Hubble Space Telescope. Wide Field Camera images of random fields have been taken in "parallel mode" with an effective...
An imaging K-band survey - I: The catalogue, star and galaxy counts (1993)
Glazebrook, Karl, Peacock, J. A., Collins, C. A., Miller, L.
We present results from a large area (552\,\sqamin) imaging $K$-band survey to a 5$\sigma$ limit of $K\simeq 17.3$. We have optical-infrared colours of almost all the objects in the sample....
Galaxies at moderate redshift (1993)
Colless, Matthew, Glazebrook, Karl, Ellis, R.S., Broadhurst, T.J., Chincarini, Guido L., Iovino, Angela, ...
We discuss the results of a series of redshift surveys of faint galaxies and their implications for galaxy evolution. In particular we address the luminosity evolution of bright galaxies at Z~1 and...
Galaxies at moderate redshift (1993)
Colless, Matthew, Glazebrook, Karl, Ellis, R.S., Broadhurst, T.J.
We discuss the results of a series of redshift surveys of faint galaxies and their implications for galaxy evolution. In particular we address the luminosity evolution of bright galaxies at Z~1 and...
Galaxies at moderate redshift (1993)
Colless, Matthew, Glazebrook, Karl, Ellis, R.S., Broadhurst, T.J.
We discuss the results of a series of redshift surveys of faint galaxies and their implications for galaxy evolution. In particular we address the luminosity evolution of bright galaxies at Z~1 and...