Detection of pairwise kSZ effect with DESI galaxy clusters and Planck

• Published in: Monthly notices of the Royal Astronomical Society 2022-03, Vol.510 (4), p.5916-5928
• Main Authors: Chen, Ziyang, Zhang, Pengjie, Yang, Xiaohu, Zheng, Yi
• Format: Article
• Language: English
• Subjects: Cluster analysis; Covariance matrix; Data analysis; Galactic clusters; Kinematics; Maximum likelihood estimators; Optical thickness; Red shift; Sky surveys (astronomy); Systematic errors
• ISSN: 0035-8711; 1365-2966
• DOI: 10.1093/mnras/stab3604

ABSTRACT We report a 5σ detection of the pairwise kinematic Sunyaev–Zel’dovich (kSZ) effect, combining galaxy clusters in DESI imaging surveys and the Planck temperature maps. The detection is facilitated by both improvements in the data and in the analysis method. For the data, we adopt the recently released DESI galaxy group catalog with ∼106 robustly identified groups, and construct various galaxy cluster samples for the kSZ measurement. The DESI group catalogue also provides estimation of halo mass, which further improves the kSZ measurement by $\sim 10{{\ \rm per\ cent}}$. For the analysis method, we derive an optimal estimator of pairwise kSZ through the maximum likelihood analysis. It also handles potential systematic errors self-consistently. The baseline cluster sample, containing the 1.2 × 105 richest galaxy clusters of typical mass ∼1014 M⊙/h at typical redshift 0.2–0.5, rules out the null hypothesis at 5σ. When fitting with a pairwise kSZ template from simulations, the signal is detected at 4.7σ and the average optical depth is constrained as $\bar{\tau }_e=(1.66\pm 0.35)\times 10^{-4}$. We perform various internal checks, with different cluster selection criteria, different sky coverage, and redshift range, different CMB maps, different filter sizes, different treatments of potential systematics, and the covariance matrix. The kSZ effect is consistently detected with 2.5 ≤S/N≤5.6 and acceptable $\chi ^2_{\rm min}$, across a variety of cluster samples. The S/N is limited by both the Planck resolution and the photo-z accuracy, and therefore, can be significant improved with DESI spectroscopic redshift information and with other CMB experiments.