Baryon content in a sample of 91 galaxy clusters selected by the South Pole Telescope at 0.2 <z < 1.25

We estimate total mass (M_500), intracluster medium (ICM) mass (M_ICM), and stellar mass (M_⋆) in a Sunyaev–Zel’dovich effect (SZE) selected sample of 91 galaxy clusters with masses M_500 ≳ 2.5 × 10^14 M_⊙ and redshift 0.2

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2018-08, Vol.478 (3), p.3072-3099
Hauptverfasser:	Chiu, I, Mohr, J J, McDonald, M, Bocquet, S, Desai, S, Klein, M, Israel, H, Ashby, M L N, Stanford, A, Benson, B A, Brodwin, M, Abbott, T M C, Abdalla, F B, Allam, S, Annis, J, Bayliss, M, Benoit-Lévy, A, Bertin, E, Bleem, L, Brooks, D, Buckley-Geer, E, Bulbul, E, Capasso, R, Carlstrom, J E, Rosell, A Carnero, Carretero, J, Castander, F J, Cunha, C E, D’Andrea, C B, da Costa, L N, Davis, C, Diehl, H T, Dietrich, J P, Doel, P, Drlica-Wagner, A, Eifler, T F, Evrard, A E, Flaugher, B, García-Bellido, J, Garmire, G, Gaztanaga, E, Gerdes, D W, Gonzalez, A, Gruen, D, Gruendl, R A, Gschwend, J, Gupta, N, Gutierrez, G, Hlavacek-L, J, Honscheid, K, James, D J, Jeltema, T, Kraft, R, Krause, E, Kuehn, K, Kuhlmann, S, Kuropatkin, N, Lahav, O, Lima, M, Maia, M A G, Marshall, J L, Melchior, P, Menanteau, F, Miquel, R, Murray, S, Nord, B, Ogando, R L C, Plazas, A A, Rapetti, D, Reichardt, C L, Romer, A K, Roodman, A, Sanchez, E, Saro, A, Scarpine, V, Schindler, R, Schubnell, M, Sharon, K, Smith, R C, Smith, M, Soares-Santos, M, Sobreira, F, Stalder, B, Stern, C, Strazzullo, V, Suchyta, E, Swanson, M E C, Tarle, G, Vikram, V, Walker, A R, Weller, J, Zhang, Y
Format:	Artikel
Sprache:	eng
Schlagworte:	ASTRONOMY AND ASTROPHYSICS Astrophysics baryon fraction clusters galaxies ICM masses Physics scaling relations stellar masses
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Beschreibung
Zusammenfassung:	We estimate total mass (M_500), intracluster medium (ICM) mass (M_ICM), and stellar mass (M_⋆) in a Sunyaev–Zel’dovich effect (SZE) selected sample of 91 galaxy clusters with masses M_500 ≳ 2.5 × 10^14 M_⊙ and redshift 0.2
ISSN:	0035-8711 1365-2966
DOI:	10.1093/mnras/sty1284