Schiappucci, E., Bianchini, F., Aguena, M., Archipley, M., Balkenhol, L., Bleem, L.E., Chaubal, P., Crawford, T.M., Grandis, S., Omori, Y., Reichardt, C.L., Rozo, E., Rykoff, E.S., To, C., Abbott, T.M.C., Ade, Peter ![]() ![]() ![]() |
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Abstract
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 4.1 σ 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 ∼ 1 , 400 deg 2 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 ¯ τ e = ( 2.97 ± 0.73 ) × 10 − 3 , while that inferred from the thermal SZ signal is ¯ τ e = ( 2.51 ± 0.5 5 stat ± 0.1 5 syst ) × 10 − 3 . The two measures agree at 0.6 σ . We perform a suite of systematic checks to test the robustness of the analysis.
Item Type: | Article |
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Date Type: | Published Online |
Status: | Published |
Schools: | Physics and Astronomy |
Publisher: | American Physical Society |
ISSN: | 2470-0010 |
Date of First Compliant Deposit: | 29 March 2023 |
Date of Acceptance: | 12 December 2022 |
Last Modified: | 04 May 2023 12:28 |
URI: | https://orca.cardiff.ac.uk/id/eprint/158178 |
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