Mass estimation of the very massive galaxy cluster SRGe CL2305.2\(-\)2248 from strong lensing

• Published in: arXiv.org 2022-04
• Main Authors: Khamitov, I M, Bikmaev, I F, Lyskova, N S, Kruglov, A A, Burenin, R A, Gilfanov, M R, Grokhovskaya, A A, Dodonov, S N, S Yu Sazonov, Starobinsky, A A, Sunyaev, R A, Khabibullin, I I, Churazov, E M
• Format: Article
• Language: English
• Subjects: Cosmology; Density distribution; Galactic clusters; Galaxies; Hubble Space Telescope; Red shift; Space telescopes; Stars & galaxies
• ISSN: 2331-8422

The galaxy cluster SRGe CL2305.2\(-\)2248 (SPT-CL J2305\(-\)2248, ACT-CL J2305.1\(-\)2248) is one of the most massive clusters at high redshifts (\(z \simeq 0.76\)) and is of great interest for cosmology. For an optical identification of this cluster, deep images were obtained with the 1.5-m Russian-Turkish telescope RTT-150. Together with the open archival data of the Hubble Space Telescope, it became possible to identify candidates for gravitationally lensed images of distant blue galaxies in the form of arcs and arclets. The observed giant arc near the brightest cluster galaxies allowed us to estimate the radius of the Einstein ring, which is \( 9.8 \pm 1.3 \) arcseconds. The photometric redshift of the lensed source was obtained (\( z_s = 2.44 \pm 0.07 \)). Its use in combination with the Einstein radius estimate made it possible to independently estimate the \cl2305 mass. It was done by extrapolating the strong lensing results to large radii and using the model density distribution profiles in relaxed clusters. This extrapolation leads to mass estimates \( \sim 1.5-3 \) times smaller than those obtained from X-ray and microwave observations. A probable cause for this discrepancy may be the process of cluster merging, which is also confirmed by SRGe CL2305.2-2248 morphology in the optical range.