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The high-mass end of the red sequence at z similar to 0.55 from SDSS-III/BOSS: completeness, bimodality and luminosity function

文献类型:期刊论文

作者Montero-Dorta, Antonio D.2; Bolton, Adam S.2,3; Brownstein, Joel R.2; Swanson, Molly1; Dawson, Kyle2; Prada, Francisco4,5,6; Eisenstein, Daniel1; Maraston, Claudia7; Thomas, Daniel7; Comparat, Johan5,6
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2016-09-11
卷号461期号:2页码:1131-1153
ISSN号0035-8711
关键词Methods: Analytical Methods: Statistical Surveys Galaxies: Evolution Galaxies: Luminosity Function, Mass Function Galaxies: Statistics
DOI10.1093/mnras/stw1352
英文摘要We have developed an analytical method based on forward-modelling techniques to characterize the high-mass end of the red sequence (RS) galaxy population at redshift z similar to 0.55, from the DR10 BOSS (Baryon Oscillation Spectroscopic Survey) CMASS spectroscopic sample, which comprises similar to 600 000 galaxies. The method, which follows an unbinned maximum likelihood approach, allows the deconvolution of the intrinsic CMASS colour-colour-magnitude distributions from photometric errors and selection effects. This procedure requires modelling the covariance matrix for the i-band magnitude, g - r colour and r - i colour using Stripe 82 multi-epoch data. Our results indicate that the error-deconvolved intrinsic RS distribution is consistent, within the photometric uncertainties, with a single point (< 0.05 mag) in the colour-colour plane at fixed magnitude, for a narrow redshift slice. We have computed the high-mass end (M-0.55(i) less than or similar to -22) of the (0.55)i-band RS luminosity function (RS LF) in several redshift slices within the redshift range 0.52 < z < 0.63. In this narrow redshift range, the evolution of the RS LF is consistent, within the uncertainties in the modelling, with a passively evolving model with Phi(*) = (7.248 +/- 0.204) x 10(-4) Mpc(-3) mag(-1), fading at a rate of 1.5 +/- 0.4 mag per unit redshift. We report RS completeness as a function of magnitude and redshift in the CMASS sample, which will facilitate a variety of galaxy-evolution and clustering studies using BOSS. Our forward-modelling method lays the foundations for future studies using other dark-energy surveys like the Extended Baryon Oscillation Spectroscopic Survey or the Dark Energy Spectroscopic Instrument, which are affected by the same type of photometric blurring/selection effects.
WOS研究方向Astronomy & Astrophysics
语种英语
出版者OXFORD UNIV PRESS
WOS记录号WOS:000383273600001
源URL[http://119.78.226.72/handle/331011/32777]  
专题中国科学院上海天文台
通讯作者Montero-Dorta, Antonio D.
作者单位1.Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
2.Univ Utah, Dept Phys & Astron, 115 South 1400 East, Salt Lake City, UT 84112 USA
3.Natl Opt Astron Observ, 950 N Cherry Ave, Tucson, AZ 85719 USA
4.CSIC, Inst Astrofis Andalucia, E-18008 Granada, Spain
5.Univ Autonoma Madrid, CSIC, Campus Int Excellence, E-28049 Madrid, Spain
6.Univ Autonoma Madrid, CSIC, Inst Fis Teor, E-28049 Madrid, Spain
7.Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg, Portsmouth PO1 3FX, Hants, England
8.Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, Shanghai 200030, Peoples R China
9.Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
10.Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA
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GB/T 7714
Montero-Dorta, Antonio D.,Bolton, Adam S.,Brownstein, Joel R.,et al. The high-mass end of the red sequence at z similar to 0.55 from SDSS-III/BOSS: completeness, bimodality and luminosity function[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2016,461(2):1131-1153.
APA Montero-Dorta, Antonio D..,Bolton, Adam S..,Brownstein, Joel R..,Swanson, Molly.,Dawson, Kyle.,...&Schneider, Donald P..(2016).The high-mass end of the red sequence at z similar to 0.55 from SDSS-III/BOSS: completeness, bimodality and luminosity function.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,461(2),1131-1153.
MLA Montero-Dorta, Antonio D.,et al."The high-mass end of the red sequence at z similar to 0.55 from SDSS-III/BOSS: completeness, bimodality and luminosity function".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 461.2(2016):1131-1153.

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