Gravity-selected cluster samples: a new take on the Compton Y-mass relation
S. Andreon, M. Radovich

TL;DR
This study examines the relation between the Compton Y parameter and galaxy cluster mass using a gravity-selected sample, revealing greater scatter and a second cluster population not seen in ICM-selected samples.
Contribution
It introduces a gravity-selected cluster sample to analyze the Y-mass relation, avoiding biases inherent in ICM-selected samples and identifying a new cluster population.
Findings
Broader scatter in Y-mass relation compared to ICM-selected samples.
Identification of a second population with low Y for their mass.
Approximately 13% of clusters belong to this second population.
Abstract
We investigate the scaling relation between the Compton Y parameter and mass in a gravity-selected sample of galaxy clusters, selected based on their gravitational lensing effects on background galaxies. Unlike ICM-selected samples, gravity-selected clusters do not require corrections for selection biases in intracluster medium (ICM) properties, such as Compton Y, since these properties are not used for selection. Our sample consists of 13 gravity-selected clusters with weak-lensing signal-to-noise ratios greater than 7 and redshifts in the range , drawn from the peak catalog of shear-selected clusters in Oguri et al. (2021). We determined spectroscopic redshifts using SDSS spectroscopy, derived tangential radial profiles from HSC shear data, and calculated cluster masses by fitting a Navarro, Frenk, \& White (1997) profile. Compton Y measurements were obtained from ACT…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Space Technology and Applications
