GLOBAL STAR FORMATION RATE DENSITY OVER 0.7 < z < 1.9

被引:52
作者
Shim, Hyunjin [1 ]
Colbert, James [2 ]
Teplitz, Harry [2 ]
Henry, Alaina [3 ]
Malkan, Mattew [3 ]
McCarthy, Patrick [4 ]
Yan, Lin [2 ]
机构
[1] Seoul Natl Univ, Dept Phys & Astron, FPRD, Seoul, South Korea
[2] CALTECH, Spitzer Sci Ctr, Pasadena, CA 91125 USA
[3] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
[4] Observ Carnegie Inst Washington, Pasadena, CA 91101 USA
基金
新加坡国家研究基金会;
关键词
galaxies: evolution; galaxies: high-redshift; galaxies: luminosity function; mass function; galaxies: starburst; ALPHA LUMINOSITY FUNCTION; EMISSION-LINE GALAXIES; STELLAR MASS DENSITY; LYMAN-BREAK GALAXIES; H-ALPHA; FORMATION HISTORY; HIGH-REDSHIFT; DEEP FIELD; EMITTING GALAXIES; FORMING GALAXIES;
D O I
10.1088/0004-637X/696/1/785
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We determine the global star formation rate (SFR) density at 0.7 < z < 1.9 using emission-line-selected galaxies identified in Hubble Space Telescope-Near Infrared Camera and Multi-Object Spectrograph (HST-NICMOS) grism spectroscopy observations. Observing in a pure parallel mode throughout HST Cycles 12 and 13, our survey covers similar to 104 arcmin(2) from which we select 80 galaxies with likely redshifted H alpha emission lines. In several cases, a somewhat weaker [O III] doublet emission is also detected. The Ha luminosity range of the emission-line galaxy sample is 4.4 x 10(41) < L(H alpha) < 1.5 x 10(43) erg s(-1). In this range, the luminosity function is well described by a Schechter function with phi* = ( 4.24 +/- 3.55) x 10(-3) Mpc(-3), L* = (2.88 +/- 1.58) x 10(42) erg s(-1), and alpha = -1.39 +/- 0.43. We derive a volume-averaged SFR density of 0.138 +/- 0.058 M(circle dot) yr(-1) Mpc(-3) at z = 1.4 without an extinction correction. Subdividing the redshift range, we find SFR densities of 0.088 +/- 0.056 M(circle dot) yr(-1) Mpc(-3) at z = 1.1 and 0.265 +/- 0.174 M(circle dot) yr(-1) Mpc(-3) at z = 1.6. The overall star formation rate density is consistent with previous studies using Ha when the same average extinction correction is applied, confirming that the cosmic peak of star formation occurs at z > 1.5.
引用
收藏
页码:785 / 796
页数:12
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Tresse, L ;
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Treyer, M ;
Bardelli, S ;
Budavari, T ;
Wyder, TK ;
Zucca, E ;
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Martin, DC ;
Vettolani, G ;
Adami, C ;
Arnaboldi, M ;
Barlow, T ;
Bianchi, L ;
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Byun, YI ;
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Charlot, S ;
Contini, T ;
Donas, J ;
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Meneux, B ;
Merighi, R ;
Morrissey, P ;
Neff, S ;
Paltani, S ;
Pellò, R .
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Zanichelli, A. ;
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Contini, T. ;
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Guzzo, L. ;
Ilbert, O. ;
Iovino, A. ;
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Pello, R. ;
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Pozzetti, L. ;
Radovich, M. ;
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Hatziminaoglou, E. ;
Polletta, M. ;
Bondi, M. ;
Brinchmann, J. ;
Cucciati, O. ;
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Gregorini, L. .
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Tremonti, C ;
Kauffmann, G ;
Heckman, T ;
Brinkmann, J .
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Yan, L ;
Chen, HW ;
Stern, D ;
Kennicutt, R ;
Spinrad, H ;
Dawson, S .
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Renzini, A ;
Cimatti, A ;
Zamorani, G ;
Menci, N ;
Daddi, E ;
Giallongo, E ;
Mignoli, M ;
Perna, C ;
Salimbeni, S ;
Saracco, P ;
Broadhurst, T ;
Cristiani, S ;
D'Odorico, S ;
Gilmozzi, R .
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