학술논문
LoVoCCS -- II. Weak Lensing Mass Distributions, Red-Sequence Galaxy Distributions, and Their Alignment with the Brightest Cluster Galaxy in 58 Nearby X-ray-Luminous Galaxy Clusters
Document Type
Working Paper
Author
Fu, Shenming; Dell'Antonio, Ian; Escalante, Zacharias; Nelson, Jessica; Englert, Anthony; Helhoski, Søren; Shinde, Rahul; Brockland, Julia; LaDuca, Philip; Larkin, Christelyn; Paris, Lucca; Weiner, Shane; Black, William K.; Chary, Ranga-Ram; Clowe, Douglas; Cooper, M. C.; Donahue, Megan; Evrard, August; Lacy, Mark; Lauer, Tod; Liu, Binyang; McCleary, Jacqueline; Meneghetti, Massimo; Miyatake, Hironao; Montes, Mireia; Natarajan, Priyamvada; Ntampaka, Michelle; Pierpaoli, Elena; Postman, Marc; Sohn, Jubee; Turner, David; Umetsu, Keiichi; Utsumi, Yousuke; Wilson, Gillian
Source
Subject
Language
Abstract
The Local Volume Complete Cluster Survey (LoVoCCS) is an on-going program to observe nearly a hundred low-redshift X-ray-luminous galaxy clusters (redshifts $0.0310^{44}$ erg/s) with the Dark Energy Camera (DECam), capturing data in $u,g,r,i,z$ bands with a $5\sigma$ point source depth of approximately 25-26th AB magnitudes. Here, we map the aperture masses in 58 galaxy cluster fields using weak gravitational lensing. These clusters span a variety of dynamical states, from nearly relaxed to merging systems, and approximately half of them have not been subject to detailed weak lensing analysis before. In each cluster field, we analyze the alignment between the 2D mass distribution described by the aperture mass map, the 2D red-sequence (RS) galaxy distribution, and the brightest cluster galaxy (BCG). We find that the orientations of the BCG and the RS distribution are strongly aligned throughout the interiors of the clusters: the median misalignment angle is 19 deg within 2 Mpc. We also observe the alignment between the orientations of the RS distribution and the overall cluster mass distribution (by a median difference of 32 deg within 1 Mpc), although this is constrained by galaxy shape noise and the limitations of our cluster sample size. These types of alignment suggest long-term dynamical evolution within the clusters over cosmic timescales.
Comment: 40 pages, 16 figures, 5 tables. Submitted to ApJ. Comments are welcome and appreciated
Comment: 40 pages, 16 figures, 5 tables. Submitted to ApJ. Comments are welcome and appreciated