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Title: Measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel’dovich effect with SPT-3G and DES

Journal Article · · Physical Review. D.
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  1. Univ. of Melbourne, VIC (Australia); SPT-3G Collaboration et al.; DES Collaboration et al.

Here, we infer the mean optical depth of a sample of optically selected galaxy clusters from the Dark Energy Survey via the pairwise kinematic Sunyaev-Zel'dovich (KSZ) effect. The pairwise KSZ signal between pairs of clusters drawn from the Dark Energy Survey Year-3 cluster catalog is detected at 4.1σ in cosmic microwave background temperature maps from two years of observations with the SPT-3G camera on the South Pole Telescope. After cuts, there are 24,580 clusters in the similar to ~1,400 deg2 of the southern sky observed by both experiments. We infer the mean optical depth of the cluster sample with two techniques. The optical depth inferred from the pairwise KSZ signal is $$\overline{τ}$$e= (2.97 ± 0.73) x 10-3, while that inferred from the thermal SZ signal is $$\overline{τ}$$e= (2.51 ± 0.55stat ± 0.15syst) x 10-3. The two measures agree at 0.6 sigma. We perform a suite of systematic checks to test the robustness of the analysis.

Research Organization:
Argonne National Laboratory (ANL), Argonne, IL (United States); Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF)
Contributing Organization:
SPT-3G Collaboration; DES Collaboration
Grant/Contract Number:
AC02-06CH11357; AC02-05CH11231; AC02- 07CH11359; De-AC02- 07CH11359; AC02-07CH11359; AC05-00OR22725
OSTI ID:
1991373
Alternate ID(s):
OSTI ID: 1960329; OSTI ID: 1994646
Journal Information:
Physical Review. D., Vol. 107, Issue 4; ISSN 2470-0010
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English

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