Environment-based selection effects of Planck clusters

被引:2
作者
Kosyra, R. [1 ,2 ]
Gruen, D. [1 ,2 ]
Seitz, S. [1 ,2 ]
Mana, A. [1 ,2 ]
Rozo, E. [3 ,4 ]
Rykoff, E. [3 ]
Sanchez, A. [2 ]
Bender, R. [1 ,2 ]
机构
[1] Univ Munich, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany
[2] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
[3] SLAC Natl Accelerator Lab, Menlo Pk, CA 94025 USA
[4] Univ Arizona, Dept Phys, Tucson, AZ 85721 USA
关键词
galaxies: clusters: general; cosmology: observations; OSCILLATION SPECTROSCOPIC SURVEY; DISCRETE OBJECT DETECTION; FAST BAYESIAN-APPROACH; WEAK LENSING ANALYSIS; GRAVITATIONAL DISTORTIONS; GALAXY CLUSTERS; X-RAY; MASS; INVERSION; CATALOG;
D O I
10.1093/mnras/stv1362
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate whether the large-scale structure environment of galaxy clusters imprints a selection bias on Sunyaev-Zel'dovich (SZ) catalogues. Such a selection effect might be caused by line of sight (LoS) structures that add to the SZ signal or contain point sources that disturb the signal extraction in the SZ survey. We use the Planck PSZ1 union catalogue in the Sloan Digital Sky Survey (SDSS) region as our sample of SZ-selected clusters. We calculate the angular two-point correlation function (2pcf) for physically correlated, foreground and background structure in the RedMaPPer SDSS DR8 catalogue with respect to each cluster. We compare our results with an optically selected comparison cluster sample and with theoretical predictions. In contrast to the hypothesis of no environment-based selection, we find a mean 2pcf for background structures of -0.049 on scales of less than or similar to 40 arcmin, significantly non-zero at similar to 4 sigma, which means that Planck clusters are more likely to be detected in regions of low background density. We hypothesize this effect arises either from background estimation in the SZ survey or from radio sources in the background. We estimate the defect in SZ signal caused by this effect to be negligibly small, of the order of similar to 10(-4) of the signal of a typical Planck detection. Analogously, there are no implications on X-ray mass measurements. However, the environmental dependence has important consequences for weak lensing follow up of Planck galaxy clusters: we predict that projection effects account for half of the mass contained within a 15 arcmin radius of Planck galaxy clusters. We did not detect a background underdensity of CMASS LRGs, which also leaves a spatially varying redshift dependence of the Planck SZ selection function as a possible cause for our findings.
引用
收藏
页码:2353 / 2366
页数:14
相关论文
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