Comparing gravitational redshifts of SDSS galaxy clusters with the magnified redshift enhancement of background BOSS galaxies

被引:26
作者
Jimeno, Pablo [1 ]
Broadhurst, Tom [1 ,2 ]
Coupon, Jean [3 ]
Umetsu, Keiichi [4 ]
Lazkoz, Ruth [1 ]
机构
[1] Univ Basque Country UPV EHU, Dept Theoret Phys & Hist Sci, E-48040 Bilbao, Spain
[2] Basque Fdn Sci, IKERBASQUE, E-48008 Bilbao, Spain
[3] Univ Geneva, Astron Observ, CH-1290 Versoix, Switzerland
[4] Acad Sinica, Inst Astron & Astrophys, Taipei 10617, Taiwan
基金
美国国家科学基金会; 美国安德鲁·梅隆基金会;
关键词
gravitational lensing: weak; galaxies: clusters: general; cosmology: observations; dark matter; DIGITAL SKY SURVEY; VLT DEEP SURVEY; LENSING ANALYSIS; DARK-MATTER; LUMINOSITY FUNCTION; DATA RELEASE; X-RAY; MASS; MAGNIFICATION; PROFILES;
D O I
10.1093/mnras/stv117
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A clean measurement of the evolution of the galaxy cluster mass function can significantly improve our understanding of cosmology from the rapid growth of cluster masses below z < 0.5. Here, we examine the consistency of cluster catalogues selected from the Sloan Digital Sky Survey by applying two independent gravity-based methods using all available spectroscopic redshifts from the DR10 release. First, we detect a gravitational redshift related signal for 20,119 and 13,128 clusters with spectroscopic redshifts contained in the Gaussian Mixture Brightest Cluster Galaxy (GMBCG) and red-sequence Matched-filter Probabilistic Percolation (redMaPPer) catalogues, respectively, at a level of similar to-10 km s(-1). This we show is consistent with the magnitude expected using the richness-mass relations provided by the literature and after applying recently clarified relativistic and flux bias corrections. This signal is also consistent with the richest clusters in the larger catalogue of Wen et al., corresponding to M-200m greater than or similar to 2 x 10(14)M(circle dot) h(-1); however, we find no significant detection of a gravitational redshift signal for lower richness clusters, which may be related to bulk motions from substructure and spurious cluster detections. Secondly, we find all three catalogues generate mass-dependent levels of lensing magnification bias, which enhances the mean redshift of flux-selected background galaxies from the Baryon Oscillation Spectroscopic Survey survey. The magnitude of this lensing effect is generally consistent with the corresponding richness-mass relations advocated for the surveys. We conclude that all catalogues comprise a high proportion of reliable clusters, and that the GMBCG and redMaPPer cluster finder algorithms favour more relaxed clusters with a meaningful gravitational redshift signal, as anticipated by the red-sequence colour selection of the GMBCG and redMaPPer samples.
引用
收藏
页码:1999 / 2012
页数:14
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