The SDSS u-band Galaxy Survey: Luminosity functions and evolution

• Published in: Monthly notices of the Royal Astronomical Society 2005-01, Vol.358
• Main Authors: Baldry, Ivan K, Glazebrook, K, Budavari, T, Eisenstein, D J, Annis, J, Bahcall, N A, Blanton, M R, Brinkmann, J, Csabai, I, Heckman, T M, Lin, H, Loveday, J, Nichol, R C, Schneider, D P, /Johns Hopkins U. /Arizona U., Astron. Dept. - Steward Observ. /Fermilab /Princeton U. /CCPP, New York /Apache Point Observ. /Eotvos U. /Sussex U.,Astron. Ctr. /Portsmouth U., ICG /Penn State U., Astron. Astrophys
• Format: Article
• Language: English
• Subjects: APERTURES; Astrophysics; ATTENUATION; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; DUSTS; GALAXIES; LUMINOSITY; STARS; WAVELENGTHS
• ISSN: 0035-8711; 1365-2966

We construct and analyze a u-band selected galaxy sample from the SDSS Southern Survey, which covers 275 deg{sup 2}. The sample includes 43223 galaxies with spectroscopic redshifts in the range 0.005 < z < 0.3 and with 14.5 < u < 20.5. The S/N in the u-band Petrosian aperture is improved by coadding multiple epochs of imaging data and by including sky-subtraction corrections. Luminosity functions for the near-UV {sup 0.1}u band ({lambda} {approx} 322 {+-} 26 nm) are determined in redshift slices of width 0.02, which show a highly significant evolution in M* of -0.8 {+-} 0.1 mag between z = 0 and 0.3; with M* - 5 log h{sub 70} = -18.84 {+-} 0.05 (AB mag), log {phi}* = -2.06 {+-} 0.03 (h{sub 70}{sup 3} Mpc{sup -3}) and log {rho}{sub L} = 19.11 {+-} 0.02 (h{sub 70} W Hz{sup -1}Mpc{sup -3}) at z = 0.1. The faint-end slope determined for z < 0.06 is given by {alpha} = -1.05 {+-} 0.08. This is in agreement with recent determinations from GALEX at shorter wavelengths. Comparing our z < 0.3 luminosity density measurements with 0.2 < z < 1.2 from COMBO-17, we find that the 280-nm density evolves as {rho}{sub L} {proportional_to} (1+z){sup {beta}} with {beta} = 2.1 {+-} 0.2; and find no evidence for any change in slope over this redshift range. By comparing with other measurements of cosmic star formation history, we estimate that the effective dust attenuation at 280 nm has increased by 0.8 {+-} 0.3 mag between z = 0 and 1.