PLCKESZ G292.51+21.98 , the SIMBAD biblio

PLCKESZ G292.51+21.98 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST03:28:22


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Title First 3 Authors
2011A&A...536A...7P viz 15       D               1 1116 260 Planck early results. VII. The Early Release Compact Source Catalogue. PLANCK COLLABORATION, ADE P.A.R., AGHANIM N., et al.
2011A&A...536A...8P viz 15       D               1 200 362 Planck early results. VIII. The all-sky early Sunyaev-Zeldovich cluster sample. PLANCK COLLABORATION, ADE P.A.R., AGHANIM N., et al.
2013ApJ...771..137M viz 15       D               1 177 9 WMAP observations of Planck ESZ clusters. MA Y.-Z., HINSHAW G. and SCOTT D.
2013A&A...555A..30B viz 38           X         1 33 28 The extended ROSAT-ESO flux limited X-ray galaxy cluster survey (REFLEX II). II. Construction and properties of the survey. BOEHRINGER H., CHON G., COLLINS C.A., et al.
2015MNRAS.450.2261M viz 16       D               1 321 30 The galaxy cluster outskirts probed by Chandra. MORANDI A., SUN M., FORMAN W., et al.
2015MNRAS.450.3665S viz 16       D               1 430 35 CoMaLit - III. Literature catalogues of weak lensing clusters of galaxies (LC2). SERENO M.
2017ApJ...843...76A viz 16       D               2 217 77 The fraction of cool-core clusters in X-ray versus SZ samples using Chandra observations. ANDRADE-SANTOS F., JONES C., FORMAN W.R., et al.
2017ApJ...846...51L 16       D               1 127 77 X-ray morphological analysis of the Planck ESZ clusters. LOVISARI L., FORMAN W.R., JONES C., et al.
2020ApJ...892..102L viz 16       D               1 121 41 X-ray scaling relations for a representative sample of Planck-selected clusters observed with XMM-Newton. LOVISARI L., SCHELLENBERGER G., SERENO M., et al.
2021ApJ...914...58A viz 17       D               1 184 9 Chandra observations of the Planck early Sunyaev-Zeldovich sample: a reexamination of masses and mass proxies. ANDRADE-SANTOS F., PRATT G.W., MELIN J.-B., et al.
2023A&A...674A..48W viz 17       D               1 120 5 Constraining the mass and redshift evolution of the hydrostatic mass bias using the gas mass fraction in galaxy clusters. WICKER R., DOUSPIS M., SALVATI L., et al.

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