GALEX-SDSS Catalogs for Statistical Studies (2009)
Budavari, T., Heinis, S., Szalay, A. S., Nieto-Santisteban, M., Gupchup, J., Shiao, B., ...
We present a detailed study of the Galaxy Evolution Explorer's photometric catalogs with special focus on the statistical properties of the All-sky and Medium Imaging Surveys. We introduce the...
Cosmological Constraints from the SDSS Luminous Red Galaxies (2006)
Tegmark, M, Eisenstein, D, Strauss, M, Weinberg, D, Blanton, M, Frieman, J, ...
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...
Galaxy bimodality versus stellar mass and environment (2006)
Baldry, I. K., Balogh, M. L., Bower, R. G., Glazebrook, K., Nichol, R. C., Bamford, S. P., ...
We analyse a z
GalICS V : Low and high order clustering in mock SDSS's (2006)
Blaizot, J., Szapudi, I., Colombi, S., Budavari, T., Bouchet, F. R., Devriendt, J. E. G., ...
[Abridged] We use mock catalogues based on the GALICS model (Hatton et al. 03) to explore the nature of galaxy clustering observed in the SDSS. We measure low and high order angular clustering...
Schiminovich, D., Ilbert, O., Arnouts, S., Milliard, B., Tresse, L., Fevre, O. Le, ...
In a companion paper (Arnouts et al. 2004) we presented new measurements of the galaxy luminosity function at 1500 Angstroms out to z~1 using GALEX-VVDS observations (1039 galaxies with NUV0.2) and...
Treyer, M., Wyder, T., Schiminovich, D., Arnouts, S., Budavari, T., Milliard, B., ...
We present measurements of the FUV (1530A) and NUV (2310A) galaxy luminosity functions (LF) at low redshift (z
Budavari, T., Szalay, A. S., Charlot, S., Seibert, M., Wyder, T. K., Arnouts, S., ...
We present measurements of the UV galaxy luminosity function and the evolution of luminosity density from GALEX observations matched to the Sloan Digital Sky Survey (SDSS). We analyze galaxies in the...
The GALEX-VVDS Measurement of the Evolution of the 1500A Luminosity Function (2005)
Arnouts, S., Schiminovich, D., Ilbert, O., Tresse, L., Milliard, B., Treyer, M., ...
We present the first measurement of the galaxy luminosity function at 1500A between 0.2
The SDSS u-band Galaxy Survey: Luminosity functions and evolution (2005)
Baldry, I. K., Glazebrook, K., Budavari, T., Eisenstein, D. J., Annis, J., Bahcall, N. A., ...
We construct and analyze a u-band selected galaxy sample from the SDSS Southern Survey, which covers 275 sq. deg. The sample includes 43223 galaxies with spectroscopic redshifts in the range 0.005
Arnouts, S., Schiminovich, D., Ilbert, O., Tresse, L., Milliard, B., Treyer, M., ...
We present the first measurement of the galaxy luminosity function (LF) at 1500 Å in the range 0.2
The GALEX-VVDS Measurement of the Evolution of the 1500A Luminosity Function (2004)
Arnouts, S., Schiminovich, D., Ilbert, O., Tresse, L., Milliard, B., Treyer, M., ...
We present the first measurement of the galaxy luminosity function at 1500A between 0.2
Schiminovich, D., Ilbert, O., Arnouts, S., Milliard, B., Tresse, L., Fevre, O. Le, ...
In a companion paper (Arnouts et al. 2004) we presented new measurements of the galaxy luminosity function at 1500 Angstroms out to z~1 using GALEX-VVDS observations (1039 galaxies with NUV0.2) and...
Budavari, T., Szalay, A. S., Charlot, S., Seibert, M., Wyder, T. K., Arnouts, S., ...
We present measurements of the UV galaxy luminosity function and the evolution of luminosity density from GALEX observations matched to the Sloan Digital Sky Survey (SDSS). We analyze galaxies in the...
Treyer, M., Wyder, T., Schiminovich, D., Arnouts, S., Budavari, T., Milliard, B., ...
We present measurements of the FUV (1530A) and NUV (2310A) galaxy luminosity functions (LF) at low redshift (z
Schiminovich, D., Ilbert, O., Arnouts, S., Milliard, B., Tresse, L., Fevre, O. Le, ...
In a companion paper (Arnouts et al. 2004) we presented new measurements of the galaxy luminosity function at 1500 Angstroms out to z~1 using GALEX-VVDS observations (1039 galaxies with NUV0.2) and...
Treyer, M., Wyder, T., Schiminovich, D., Arnouts, S., Budavari, T., Milliard, B., ...
We present measurements of the FUV (1530A) and NUV (2310A) galaxy luminosity functions (LF) at low redshift (z
Budavari, T., Szalay, A. S., Charlot, S., Seibert, M., Wyder, T. K., Arnouts, S., ...
We present measurements of the UV galaxy luminosity function and the evolution of luminosity density from GALEX observations matched to the Sloan Digital Sky Survey (SDSS). We analyze galaxies in the...
The GALEX-VVDS Measurement of the Evolution of the 1500A Luminosity Function (2004)
Arnouts, S., Schiminovich, D., Ilbert, O., Tresse, L., Milliard, B., Treyer, M., ...
We present the first measurement of the galaxy luminosity function at 1500A between 0.2
Schiminovich, D., Ilbert, O., Arnouts, S., Milliard, B., Tresse, L., Fevre, O. Le, ...
In a companion paper (Arnouts et al. 2004) we presented new measurements of the galaxy luminosity function at 1500 Angstroms out to z~1 using GALEX-VVDS observations (1039 galaxies with NUV0.2) and...
Treyer, M., Wyder, T., Schiminovich, D., Arnouts, S., Budavari, T., Milliard, B., ...
We present measurements of the FUV (1530A) and NUV (2310A) galaxy luminosity functions (LF) at low redshift (z
Budavari, T., Szalay, A. S., Charlot, S., Seibert, M., Wyder, T. K., Arnouts, S., ...
We present measurements of the UV galaxy luminosity function and the evolution of luminosity density from GALEX observations matched to the Sloan Digital Sky Survey (SDSS). We analyze galaxies in the...
The GALEX-VVDS Measurement of the Evolution of the 1500A Luminosity Function (2004)
Arnouts, S., Schiminovich, D., Ilbert, O., Tresse, L., Milliard, B., Treyer, M., ...
We present the first measurement of the galaxy luminosity function at 1500A between 0.2
The Galaxy-mass Correlation Function Measured from Weak Lensing in the SDSS (2003)
Sheldon, E. S., Johnston, D. E., Frieman, J. A., Scranton, R., McKay, T. A., Connolly, A. J., ...
We present galaxy-galaxy lensing measurements over scales 0.025 to 10 Mpc/h in the Sloan Digital Sky Survey. Using a flux-limited sample of 127,001 lens galaxies with spectroscopic redshifts and mean...
Cosmological parameters from SDSS and WMAP (2003)
Tegmark, M., Strauss, M., Blanton, M., Abazajian, K., Dodelson, S., Sandvik, H., ...
We measure cosmological parameters using the three-dimensional power spectrum P(k) from over 200,000 galaxies in the Sloan Digital Sky Survey (SDSS) in combination with WMAP and other data. Our...
The 3D power spectrum of galaxies from the SDSS (2003)
Tegmark, M, Blanton, M, Strauss, M, Hoyle, F, Schlegel, D, Scoccimarro, R, ...
We measure the large-scale real-space power spectrum P(k) using a sample of 205,443 galaxies from the Sloan Digital Sky Survey, covering 2417 square degrees with mean redshift z~0.1. We employ a...
Stanford, S. A., Dickinson, M., Postman, M., Ferguson, H., Lucas, R., Conselice, C., ...
The redshift distribution of well-defined samples of distant early-type galaxies offers a means to test the predictions of monolithic and hierarchical galaxy formation scenarios. NICMOS maps of the...
Physical Evidence for Dark Energy (2003)
Scranton, R., Connolly, A. J., Nichol, R. C., Stebbins, A., Szapudi, I., Eisenstein, D. J., ...
We present measurements of the angular cross-correlation between luminous red galaxies from the Sloan Digital Sky Survey and the cosmic microwave background temperature maps from the Wilkinson...
Reconstructing Galaxy Spectral Energy Distributions from Broadband Photometry (1999)
Csabai, I., Connolly, A. J., Szalay, A. S., Budavari, T.
We present a novel approach to photometric redshifts, one that merges the advantages of both the template fitting and empirical fitting algorithms, without any of their disadvantages. This technique...
Calibrating photometric redshifts of luminous red galaxies
Padmanabhan, N, Budavari, T, Schlegel, DJ, Bridges, T, Brinkmann, J, Cannon, R, ...
We discuss the construction of a photometric redshift catalogue of luminous red galaxies (LRGs) from the Sloan Digital Sky Survey (SDSS), emphasizing the principal steps necessary for constructing...