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X-Ray Properties of SPT-selected Galaxy Clusters at 0.2 < z < 1.5 Observed with XMM-Newton
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Resolving the hydrostatic mass profiles of galaxy clusters at z ∼ 1 with XMM-Newton and Chandra
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The FABLE simulations: a feedback model for galaxies, groups, and clusters
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Optical Follow-up of Planck Cluster Candidates with Small Instruments
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Planck Sunyaev–Zel’dovich cluster mass calibration using Hyper Suprime-Cam weak lensing
Elinor Medezinski, Nicholas Battaglia, Keiichi Umetsu, Masamune Oguri, Hironao Miyatake, Atsushi J Nishizawa, Cristóbal Sifón, David N Spergel, I-Non Chiu, Yen-Ting Lin, Neta Bahcall and Yutaka Komiyama Publications of the Astronomical Society of Japan 70(SP1) (2018) https://doi.org/10.1093/pasj/psx128
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I Chiu, J J Mohr, M McDonald, et al. Monthly Notices of the Royal Astronomical Society 478(3) 3072 (2018) https://doi.org/10.1093/mnras/sty1284
First Sunyaev–Zel’dovich mapping with the NIKA2 camera: Implication of cluster substructures for the pressure profile and mass estimate
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Substructure and merger detection in resolved NIKA Sunyaev-Zel’dovich images of distant clusters
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AMI observations of 10 CLASH galaxy clusters: SZ and X-ray data used together to determine cluster dynamical states
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The physics inside the scaling relations for X-ray galaxy clusters: gas clumpiness, gas mass fraction and slope of the pressure profile
Reconciling Planck cluster counts and cosmology? Chandra/XMM instrumental calibration and hydrostatic mass bias
Holger Israel, Gerrit Schellenberger, Jukka Nevalainen, Richard Massey and Thomas H. Reiprich Monthly Notices of the Royal Astronomical Society 448(1) 814 (2015) https://doi.org/10.1093/mnras/stv038
SUPERMODEL ANALYSIS OF A1246 AND J255: ON THE EVOLUTION OF GALAXY CLUSTERS FROM HIGH TO LOW ENTROPY STATES
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P. A. Giles, B. J. Maughan, T. Hamana, et al. Monthly Notices of the Royal Astronomical Society 447(4) 3044 (2015) https://doi.org/10.1093/mnras/stu2679
LoCuSS: Testing hydrostatic equilibrium in galaxy clusters
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LoCuSS: the near-infrared luminosity and weak-lensing mass scaling relation of galaxy clusters
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SCALING RELATIONS AND X-RAY PROPERTIES OF MODERATE-LUMINOSITY GALAXY CLUSTERS FROM 0.3
Thomas Connor, Megan Donahue, Ming Sun, et al. The Astrophysical Journal 794(1) 48 (2014) https://doi.org/10.1088/0004-637X/794/1/48
Chemical evolution on the scale of clusters of galaxies: a conundrum?
Cosmological simulations of galaxy clusters with feedback from active galactic nuclei: profiles and scaling relations
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A comparative study of local galaxy clusters – II. X-ray and SZ scaling relations
E. Rozo, A. E. Evrard, E. S. Rykoff and J. G. Bartlett Monthly Notices of the Royal Astronomical Society 438(1) 62 (2014) https://doi.org/10.1093/mnras/stt2160
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CLASH-X: A COMPARISON OF LENSING AND X-RAY TECHNIQUES FOR MEASURING THE MASS PROFILES OF GALAXY CLUSTERS
ERRATUM: “ON THE CLUSTER PHYSICS OF SUNYAEV-ZEL'DOVICH AND X-RAY SURVEYS. III. MEASUREMENT BIASES AND COSMOLOGICAL EVOLUTION OF GAS AND STELLAR MASS FRACTIONS” (2013, ApJ, 777, 123)
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Sunyaev-Zel'dovich observations with AMI of the hottest galaxy clusters detected in the XMM-Newton Cluster Survey
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MEASUREMENT OF THE DISPERSION OF RADIATION FROM A STEADY COSMOLOGICAL SOURCE
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A. K. Hicks, G. W. Pratt, M. Donahue, et al. Monthly Notices of the Royal Astronomical Society 431(3) 2542 (2013) https://doi.org/10.1093/mnras/stt348
Distribution of Si, Fe, and Ni in the Intracluster Medium of the Coma Cluster
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SOUTH POLE TELESCOPE DEEP FIELD: SURVEY DESIGN AND INFRARED ARRAY CAMERA CATALOGS