Luminosity Functions of Lyman Break Galaxies at z ~ 4 and z ~ 5 in the Subaru Deep Field

We investigate the luminosity functions of Lyman break galaxies (LBGs) at z ~ 4 and z ~ 5 based on optical imaging data obtained in the Subaru Deep Field project. Three samples of LBGs in a contiguous area of 875 arcmin2 are constructed. One consists of 3808 LBGs at z ~ 4 down to i' = 26.85 selected with the B-R versus R-i' diagram. The other two consist of 539 and 240 LBGs at z ~ 5 down to z' = 26.05 selected with two kinds of two-color diagram: V-i' versus i'-z' and R-i' versus i'-z'. The adopted selection criteria are proved to be fairly reliable by spectroscopic observations. We derive the luminosity functions of the LBGs at rest-frame ultraviolet wavelengths down to MUV = -19.2 at z ~ 4 and MUV = -20.3 at z ~ 5. We find clear evolution of the luminosity function over the redshift range 0 ≤ z ≤ 6, which is accounted for solely by a change in the characteristic magnitude M*. We examine the evolution of the cosmic star formation rate (SFR) density and its luminosity dependence over 0 ≤ z ≲ 6. The SFR density contributed from brighter galaxies is found to change more drastically with cosmic time. The contribution from brighter galaxies has a sharp peak around z = 3-4, while that from fainter galaxies evolves relatively mildly with a broad peak at earlier epochs. Combining the observed SFR density with the standard cold dark matter model, we compute the cosmic SFR per unit baryon mass in dark halos, that is, the specific SFR. The specific SFR is found to scale with redshift as (1 + z)3 up to z ~ 4, implying that the efficiency of star formation is on average higher at higher redshift in proportion to the cooling rate within dark halos, while this is not simply the case at z ≳ 4.

[1]  K. Tashima,et al.  Pharmacogenetics of plasma efavirenz exposure after treatment discontinuation: an Adult AIDS Clinical Trials Group Study. , 2006, Clinical infectious diseases : an official publication of the Infectious Diseases Society of America.

[2]  S. Mallal,et al.  Efavirenz and CYP2B6 polymorphism: implications for drug toxicity and resistance. , 2006, Clinical infectious diseases : an official publication of the Infectious Diseases Society of America.

[3]  S. Okamura,et al.  Clustering of Lyman Break Galaxies at z = 4 and 5 in the Subaru Deep Field: Luminosity Dependence of the Correlation Function Slope , 2005, astro-ph/0509564.

[4]  M. Sawicki,et al.  Keck Deep Fields. II. The Ultraviolet Galaxy Luminosity Function at z ~ 4, 3, and 2 , 2005, astro-ph/0507519.

[5]  M. Ziats,et al.  Prevalence of CYP2B6 alleles in malaria-endemic populations of West Africa and Papua New Guinea , 2006, European Journal of Clinical Pharmacology.

[6]  R. Bouwens,et al.  Galaxies at z ~ 6: The UV Luminosity Function and Luminosity Density from 506 HUDF, HUDF Parallel ACS Field, and GOODS i-Dropouts , 2005, astro-ph/0509641.

[7]  Y. Yoshii,et al.  Numerical Galaxy Catalog. I. A Semianalytic Model of Galaxy Formation with N-Body Simulations , 2005, astro-ph/0508085.

[8]  Joo-Youn Cho,et al.  HAPLOTYPE STRUCTURE AND ALLELE FREQUENCIES OF CYP2B6 IN A KOREAN POPULATION , 2004, Drug Metabolism and Disposition.

[9]  A. M. Hopkins,et al.  On the Evolution of Star-forming Galaxies , 2004, astro-ph/0407170.

[10]  S. Okamura,et al.  Subaru Deep Survey. VI. A Census of Lyman Break Galaxies at z ≃ 4 and 5 in the Subaru Deep Fields: Clustering Properties , 2003, astro-ph/0309657.

[11]  M. Giavalisco,et al.  Lyman Break Galaxies at Redshift z ~ 3: Survey Description and Full Data Set , 2003, astro-ph/0305378.

[12]  Department of Physics,et al.  accepted for publication in the Astrophysical Journal Luminous Lyman Break Galaxies at z>5 and the Source of , 2003 .

[13]  M. Hiratsuka,et al.  PHARMACOKINETICS AND DISPOSITION , 2002 .

[14]  H. Ferguson,et al.  The Stellar Populations and Evolution of Lyman Break Galaxies , 2000, astro-ph/0105087.

[15]  C. C. Steidel,et al.  Multiwavelength Observations of Dusty Star Formation at Low and High Redshift , 2000, astro-ph/0001126.

[16]  Research Center for the Early Universe,et al.  New Improved Photometric Redshifts of Galaxies in the Hubble Deep Field , 1999, astro-ph/9912447.

[17]  A. Kinney,et al.  The Dust Content and Opacity of Actively Star-forming Galaxies , 1999, astro-ph/9911459.

[18]  D. Schlegel,et al.  Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds , 1998 .