TY - JOUR
T1 - The LBT Boötes Field Survey. I. The Rest-frame Ultraviolet and Near-infrared Luminosity Functions and Clustering of Bright Lyman Break Galaxies at Z ~ 3
AU - Bian, Fuyan
AU - Fan, Xiaohui
AU - Jiang, Linhua
AU - McGreer, Ian
AU - Dey, Arjun
AU - Green, Richard F.
AU - Maiolino, Roberto
AU - Walter, Fabian
AU - Lee, Kyoung-Soo
AU - Davé, Romeel
PY - 2013/8/13
Y1 - 2013/8/13
N2 - We present a deep LBT/LBC U spec-band imaging survey (9
deg2) covering the NOAO Boötes field. A total of 14,485
Lyman break galaxies (LBGs) at z ~ 3 are selected, which are used to
measure the rest-frame UV luminosity function (LF). The large sample
size and survey area reduce the LF uncertainties due to Poisson
statistics and cosmic variance by >=3 compared to previous studies.
At the bright end, the LF shows excess power compared to the best-fit
Schechter function, which can be attributed to the contribution of z ~ 3
quasars. We compute the rest-frame near-infrared LF and stellar mass
function (SMF) of z ~ 3 LBGs based on the R-band and [4.5 μm]-band
flux relation. We investigate the evolution of the UV LFs and SMFs
between z ~ 7 and z ~ 3, which supports a rising star formation history
in the LBGs. We study the spatial correlation function of two bright LBG
samples and estimate their average host halo mass. We find a tight
relation between the host halo mass and the galaxy star formation rate
(SFR), which follows the trend predicted by the baryonic accretion rate
onto the halo, suggesting that the star formation in LBGs is fueled by
baryonic accretion through the cosmic web. By comparing the SFRs with
the total baryonic accretion rates, we find that cosmic star formation
efficiency is about 5%-20% and it does not evolve significantly with
redshift, halo mass, or galaxy luminosity.
Based on data acquired using the Large Binocular Telescope (LBT). The
LBT is an international collaboration among institutions in the United
States, Italy, and Germany. LBT Corporation partners are: The University
of Arizona on behalf of the Arizona university system; Istituto
Nazionale di Astrofisica, Italy; LBT Beteiligungsgesellschaft, Germany,
representing the Max-Planck Society, the Astrophysical Institute
Potsdam, and Heidelberg University; The Ohio State University, and The
Research Corporation, on behalf of The University of Notre Dame,
University of Minnesota, and University of Virginia.
AB - We present a deep LBT/LBC U spec-band imaging survey (9
deg2) covering the NOAO Boötes field. A total of 14,485
Lyman break galaxies (LBGs) at z ~ 3 are selected, which are used to
measure the rest-frame UV luminosity function (LF). The large sample
size and survey area reduce the LF uncertainties due to Poisson
statistics and cosmic variance by >=3 compared to previous studies.
At the bright end, the LF shows excess power compared to the best-fit
Schechter function, which can be attributed to the contribution of z ~ 3
quasars. We compute the rest-frame near-infrared LF and stellar mass
function (SMF) of z ~ 3 LBGs based on the R-band and [4.5 μm]-band
flux relation. We investigate the evolution of the UV LFs and SMFs
between z ~ 7 and z ~ 3, which supports a rising star formation history
in the LBGs. We study the spatial correlation function of two bright LBG
samples and estimate their average host halo mass. We find a tight
relation between the host halo mass and the galaxy star formation rate
(SFR), which follows the trend predicted by the baryonic accretion rate
onto the halo, suggesting that the star formation in LBGs is fueled by
baryonic accretion through the cosmic web. By comparing the SFRs with
the total baryonic accretion rates, we find that cosmic star formation
efficiency is about 5%-20% and it does not evolve significantly with
redshift, halo mass, or galaxy luminosity.
Based on data acquired using the Large Binocular Telescope (LBT). The
LBT is an international collaboration among institutions in the United
States, Italy, and Germany. LBT Corporation partners are: The University
of Arizona on behalf of the Arizona university system; Istituto
Nazionale di Astrofisica, Italy; LBT Beteiligungsgesellschaft, Germany,
representing the Max-Planck Society, the Astrophysical Institute
Potsdam, and Heidelberg University; The Ohio State University, and The
Research Corporation, on behalf of The University of Notre Dame,
University of Minnesota, and University of Virginia.
KW - galaxies: evolution
KW - galaxies: formation
KW - galaxies: high-redshift
U2 - 10.1088/0004-637X/774/1/28
DO - 10.1088/0004-637X/774/1/28
M3 - Article
SN - 0004-637X
VL - 774
SP - 28
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 1
ER -