Baryon Content of Massive Galaxy Clusters (0.57 < z < 1.33)

• Main Authors: Chiu, I., Mohr, J., Mcdonald, M., Bocquet, S., Ashby, M. L., Bayliss, M., Benson, B. A., Bleem, L. E., Brodwin, M., Desai, S., Dietrich, J. P., Forman, W. R., Gangkofner, C., Gonzalez, A. H., Hennig, C., Liu, J., Reichardt, C. L., Saro, A., Stalder, B., Stanford, S. A., Song, J., Schrabback, T., Suhada, R., Strazzullo, V., Zenteno, A.
• Format: Text
• Language: unknown
• Published: arXiv 2014
• Subjects: Cosmology and Nongalactic Astrophysics astro-ph.CO; FOS Physical sciences; Pivot; South Pole; South pole
• Online Access: https://dx.doi.org/10.48550/arxiv.1412.7823; https://arxiv.org/abs/1412.7823

We study the stellar, Brightest Cluster Galaxy (BCG) and intracluster medium (ICM) masses of 14 South Pole Telescope (SPT) selected galaxy clusters with median redshift $z=0.9$ and median mass $M_{500}=6\times10^{14}M_{\odot}$. We estimate stellar masses for each cluster and BCG using six photometri...