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Galaxy Clusters at Z 1 Imaged by ALMA with the Sunyaev-Zel'dovich Effect

Publications of the Astronomical Society of Japan(2023)

Toho Univ | Acad Sinica Inst Astron & Astrophys ASIAA | Hiroshima Univ | Natl Astron Observ Japan | Univ KwaZulu Natal | Rutgers State Univ | Rikkyo Univ | Univ Tokyo | Max Planck Inst Astrophys | Chiba Univ | Pontificia Univ Catolica Valparaiso | Yamagata Univ | Natl Radio Astron Observ | European Southern Observ ESO | NASA

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Abstract
We present high angular-resolution measurements of the thermal Sunyaev-Zel'dovich effect (SZE) toward two galaxy clusters, RCS J2319+0038 at z=0.9 and HSC J0947-0119 at z=1.1, by the Atacama Large Millimeter/submillimeter Array (ALMA) in Band 3. They are supplemented with available Chandra X-ray data, optical data taken by Hyper Suprime-Cam on Subaru, and millimeter-wave SZE data from the Atacama Cosmology Telescope. Taking into account departures from spherical symmetry, we have reconstructed non-parametrically the inner pressure profile of two clusters as well as electron temperature and density profiles for RCS J2319+0038. This is one of the first such measurements for an individual cluster at $z \gtrsim 0.9$. We find that the inner pressure profile of both clusters is much shallower than that of local cool-core clusters. Our results consistently suggest that RCS J2319+0038 hosts a weak cool core, where radiative cooling is less significant than in local cool cores. On the other hand, HSC J0947-0119 exhibits an even shallower pressure profile than RCS J2319+0038 and is more likely a non-cool-core cluster. The SZE centroid position is offset by more than 140 $h_{70}^{-1}$kpc from the peaks of galaxy distribution in HSC J0947-0119, suggesting a stronger influence of mergers in this cluster. We conclude that these distant clusters are at a very early stage of developing the cool cores typically found in clusters at lower redshifts.
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cosmology: observations,galaxies: clusters: intracluster medium,galaxies: clusters: individual (RCS J2319+0038, HSC J0947-0119),radio continuum: galaxies,techniques: interferometric
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