Baryon content of massive galaxy clusters at 0.57 < z < 1.33

• Published in: Monthly Notices of the Royal Astronomical Society
• Main Authors: Chiu, I., Mohr, J., McDonald, M., Bocquet, S., Ashby, M. L. N., 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., Šuhada, R., Strazzullo, V., Zenteno, A.
• Other Authors: Mcdonald, M.
• Format: Article in Journal/Newspaper
• Language: English
• Published: 2016
• Subjects: Cluster; Evolution; Galaxie; Galaxy; General; Large-scale structure of Universe; X-ray; Astronomy and Astrophysic; Space and Planetary Science; Pivot; South Pole; South pole
• Online Access: http://hdl.handle.net/11368/2962594; https://doi.org/10.1093/mnras/stv2303; https://academic.oup.com/mnras/article/455/1/258/984806

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 mass M500 = 6 × 1014 M☉. We estimate stellar masses for each cluster and BCG using six photometric bands, the ICM mass...