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 energy output of the Universe from 0.1 micron to 1000 micron (2008)
Driver, Simon P., Popescu, Cristina C., Tuffs, Richard J., Graham, Alister W., Liske, Jochen, Baldry, Ivan
The dominant source of electromagnetic energy in the Universe today (over ultraviolet, optical and near-infrared wavelengths) is starlight. However, quantifying the amount of starlight produced has...
The energy output of the universe from 0.1 to 1000 μm (2008)
Driver, Simon P., Popescu, Cristina C., Tuffs, Richard J., Graham, Alister W., Liske, Jochen, Baldry, Ivan
The dominant source of electromagnetic energy in the universe today (over ultraviolet, optical, and near-infrared wavelengths) is starlight. However, quantifying the amount of starlight produced has...
The energy output of the universe from 0.1 to 1000 μm (2008)
Driver, Simon P., Popescu, Cristina C., Tuffs, Richard J., Graham, Alister W., Liske, Jochen, Baldry, Ivan
The dominant source of electromagnetic energy in the universe today (over ultraviolet, optical, and near-infrared wavelengths) is starlight. However, quantifying the amount of starlight produced has...
The energy output of the universe from 0.1 to 1000 μm (2008)
Driver, Simon P., Popescu, Cristina C., Tuffs, Richard J., Graham, Alister W., Liske, Jochen, Baldry, Ivan
The dominant source of electromagnetic energy in the universe today (over ultraviolet, optical, and near-infrared wavelengths) is starlight. However, quantifying the amount of starlight produced has...
The energy output of the universe from 0.1 to 1000 μm (2008)
Driver, Simon P., Popescu, Cristina C., Tuffs, Richard J., Graham, Alister W., Liske, Jochen, Baldry, Ivan
The dominant source of electromagnetic energy in the universe today (over ultraviolet, optical, and near-infrared wavelengths) is starlight. However, quantifying the amount of starlight produced has...
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,...
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...
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...
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...
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.
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