Connecting stellar mass and star-formation rate to dark matter halo mass out to z ∼ 2

被引：74
作者：
Wang, L. [1 ,2 ]
Farrah, D. [1 ,3 ]
Oliver, S. J. [1 ]
Amblard, A. [4 ]
Bethermin, M. [5 ,6 ,7 ]
Bock, J. [8 ,9 ]
Conley, A. [10 ]
Cooray, A. [8 ,11 ]
Halpern, M. [12 ]
Heinis, S. [13 ]
Ibar, E. [14 ]
Ilbert, O. [13 ]
Ivison, R. J. [14 ,15 ]
Marsden, G. [12 ]
Roseboom, I. G. [1 ,15 ]
Rowan-Robinson, M. [16 ]
Schulz, B. [8 ,17 ]
Smith, A. J. [1 ]
Viero, M. [8 ]
Zemcov, M. [8 ,9 ]
机构：
[1] Univ Sussex, Dept Phys & Astron, Ctr Astron, Brighton BN1 9QH, E Sussex, England
[2] Univ Durham, Inst Computat Cosmol, Dept Phys, Durham DH1 3LE, England
[3] Virginia Tech, Dept Phys, Blacksburg, VA 24061 USA
[4] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[5] Univ Paris Diderot, CE Saclay, CNRS, Lab AIM Paris Saclay,CEA,DSM,Irfu, F-91191 Gif Sur Yvette, France
[6] Univ Paris 11, IAS, F-91405 Orsay, France
[7] CNRS, UMR 8617, F-91405 Orsay, France
[8] CALTECH, Pasadena, CA 91125 USA
[9] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[10] Univ Colorado, Ctr Astrophys & Space Astron UCB 389, Boulder, CO 80309 USA
[11] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA
[12] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
[13] Univ Aix Marseille, CNRS, OAMP, Lab Astrophys Marseille, F-13388 Marseille 13, France
[14] Royal Observ, UK Astron Technol Ctr, Edinburgh EH9 3HJ, Midlothian, Scotland
[15] Univ Edinburgh, Inst Astron, Royal Observ, Edinburgh EH9 3HJ, Midlothian, Scotland
[16] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Astrophys Grp, London SW7 2AZ, England
[17] CALTECH, Infrared Proc & Anal Ctr, JPL, Pasadena, CA 91125 USA
来源：
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2013年 / 431卷 / 01期
基金：
英国科学技术设施理事会;
关键词：
methods: statistical; cosmology: observations; large-scale structure of Universe; infrared: galaxies; ACTIVE GALACTIC NUCLEI; DIGITAL SKY SURVEY; SPECTRAL ENERGY-DISTRIBUTIONS; GALAXY FORMATION; PHOTOMETRIC REDSHIFTS; FORMATION HISTORY; LUMINOSITY DENSITY; COSMOS FIELD; SPITZER/IRAC SOURCES; FORMING GALAXIES;
D O I：
10.1093/mnras/stt190
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We have constructed an extended halo model (EHM) which relates the total stellar mass and star-formation rate (SFR) to halo mass (M-h). An empirical relation between the distribution functions of total stellar mass of galaxies and host halo mass, tuned to match the spatial density of galaxies over 0 < z < 2 and the clustering properties at z similar to 0, is extended to include two different scenarios describing the variation of SFR on Mh. We also present new measurements of the redshift evolution of the average SFR for star-forming galaxies of different stellar masses up to z = 2, using data from the Herschel Multi-tiered Extragalactic Survey for infrared bright galaxies. Combining the EHM with the halo accretion histories from numerical simulations, we trace the stellar mass growth and star-formation history in haloes spanning a range of masses. We find that: (1) the intensity of the star-forming activity in haloes in the probed mass range has steadily decreased from z similar to 2 to 0; (2) at a given epoch, haloes in the mass range between a few times 10(11) M-circle dot and a few times 10(12) M-circle dot are the most efficient at hosting star formation; (3) the peak of SFR density shifts to lower mass haloes over time; and (4) galaxies that are forming stars most actively at z similar to 2 evolve into quiescent galaxies in today's group environments, strongly supporting previous claims that the most powerful starbursts at z similar to 2 are progenitors of today's elliptical galaxies.
引用
收藏
页码：648 / 661
页数：14
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