The Cluster HEritage project with XMM-Newton: Mass Assembly and Thermodynamics at the Endpoint of structure formation: I. Programme overview

被引:65
作者
Arnaud, M. [1 ]
Ettori, S. [2 ,3 ]
Pratt, G. W. [1 ]
Rossetti, M. [4 ]
Eckert, D. [5 ]
Gastaldello, F. [4 ]
Gavazzi, R. [6 ,7 ]
Kay, S. T. [8 ]
Lovisari, L. [2 ,9 ]
Maughan, B. J. [10 ]
Pointecouteau, E. [11 ]
Sereno, M. [2 ,3 ]
Bartalucci, I [1 ,4 ]
Bonafede, A. [12 ,13 ,14 ]
Bourdin, H. [15 ]
Cassano, R. [13 ]
Duffy, R. T. [10 ]
Iqbal, A. [1 ]
Maurogordato, S. [16 ]
Rasia, E. [17 ,18 ]
Sayers, J. [19 ]
Andrade-Santos, F. [9 ]
Aussel, H. [1 ]
Barnes, D. J. [20 ,21 ]
Barrena, R. [22 ,23 ]
Borgani, S. [17 ,18 ,24 ,25 ]
Burkutean, S. [13 ]
Clerc, N. [11 ]
Corasaniti, P-S [26 ,27 ]
Cuillandre, J-C [1 ]
De Grandi, S. [28 ]
De Petris, M. [29 ]
Dolag, K. [30 ,31 ]
Donahue, M. [32 ]
Ferragamo, A. [29 ]
Gaspari, M. [2 ,33 ]
Ghizzardi, S. [4 ]
Gitti, M. [12 ,13 ]
Haines, C. P. [48 ]
Jauzac, M. [34 ,35 ,36 ,37 ]
Johnston-Hollitt, M. [38 ,39 ]
Jones, C. [9 ]
Keruzore, F. [40 ]
LeBrun, A. M. C. [1 ,26 ]
Mayet, F. [40 ]
Mazzotta, P. [15 ]
Melin, J-B [41 ]
Molendi, S. [4 ]
Nonino, M. [17 ]
Okabe, N. [42 ]
机构
[1] Univ Paris Diderot, Sorbonne Paris Cite, Univ Paris Saclay, AIM,CEA,CNRS, F-91191 Gif Sur Yvette, France
[2] INAF, Osservatorio Astrofis & Sci Spazio, Via Pietro Gobetti 93-3, I-40129 Bologna, Italy
[3] Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy
[4] IASF Milano, INAF, Via A Corti 12, I-20133 Milan, Italy
[5] Univ Geneva, Dept Astron, Ch Ec 16, CH-1290 Versoix, Switzerland
[6] CNRS, 98Bis Blvd Arago, F-75014 Paris, France
[7] Sorbonne Univ, UMR 7095, Inst Astrophys Paris, 98Bis Blvd Arago, F-75014 Paris, France
[8] Univ Manchester, Sch Nat Sci, Dept Phys & Astron, Jodrell Bank Ctr Astrophys, Manchester M13 9PL, Lancs, England
[9] Harvard & Smithsonian, Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[10] Univ Bristol, HH Wills Phys Lab, Tyndall Ave, Bristol BS8 1TL, Avon, England
[11] Univ Toulouse, IRAP, CNRS, CNES,UPS, 9 Av Colonel Roche,BP 44346, F-31028 Toulouse 4, France
[12] Univ Bologna, Dipartimento Fis & Astron, Via Gobetti 92-3, I-40121 Bologna, Italy
[13] Ist Radio Astron, INAF, Via Gobetti 101, I-40129 Bologna, Italy
[14] Hamburger Sternwarte, Gojenbergsweg 112, D-21029 Hamburg, Germany
[15] Univ Roma Tor Vergata, Via Ric Sci 1, I-00133 Rome, Italy
[16] Univ Cote dAzur, Observ Cote dAzur, Lab Lagrange, CNRS, Nice, France
[17] INAF Osservatorio Astron Trieste, Via Tiepolo 11, I-34131 Trieste, Italy
[18] IFPU Inst Fundamental Phys Universe, Via Beirut 2, I-34151 Trieste, Italy
[19] CALTECH, Pasadena, CA 91125 USA
[20] MIT, Dept Phys, Cambridge, MA 02139 USA
[21] MIT, Kavli Inst Astrophys & Space Res, Cambridge, MA 02139 USA
[22] Inst Astrofis Canarias IAC, C Via Lactea S-N, Tenerife 38205, Spain
[23] Univ La Laguna, Dept Astrofis, C Astrofis Francisco Sanchez S-N, Tenerife 38206, Spain
[24] Univ Trieste, Sez Astron, Dipartimento Fis, Via Tiepolo 11, I-34143 Trieste, Italy
[25] Ist Nazl Fis Nucl, Sez Trieste, I-34100 Trieste, Italy
[26] Univ Paris, PSL Res Univ, Observ Paris, LUTH,UMR 8102 CNRS, 5 Pl Jules Janssen, F-92195 Meudon, France
[27] Sorbonne Univ, Inst Astrophys Paris, CNRS, UMR 7095, 98Bis Bd Arago, F-75014 Paris, France
[28] INAF, Osservatorio Astron Brera, Via E Bianchi 46, I-23807 Merate, Italy
[29] Sapienza Univ Roma, Dipartimento Fis, Piazzale Aldo Moro 5, I-500185 Rome, Italy
[30] Univ Observ Munich, Scheinerstr 1, D-81679 Munich, Germany
[31] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85748 Garching, Germany
[32] Michigan State Univ, Phys & Astron Dept, E Lansing, MI 48824 USA
[33] Princeton Univ, Dept Astrophys Sci, 4 Ivy Lane, Princeton, NJ 08544 USA
[34] Univ Durham, Ctr Extragalact Astron, South Rd, Durham DH1 3LE, England
[35] Univ Durham, Inst Computat Cosmol, South Rd, Durham DH1 3LE, England
[36] Univ KwaZulu Natal, Astrophys Res Ctr, Westville Campus, ZA-4041 Durban, South Africa
[37] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Westville Campus, ZA-4041 Durban, South Africa
[38] Curtin Inst Computat, GPO Box U1987, Perth, WA 6845, Australia
[39] Curtin Univ, Int Ctr Radio Astron Res ICRAR, Bentley, WA 6102, Australia
[40] Univ Grenoble Alpes, CNRS, LPSC IN2P3, 53 Ave Martyrs, F-38000 Grenoble, France
[41] Univ Paris Saclay, CEA, IRFU, F-91191 Gif Sur Yvette, France
[42] Hiroshima Univ, Grad Sch Adv Sci & Engn, Phys Program, 1-3-1 Kagamiyama, Higashihiroshima, Hiroshima 7398526, Japan
[43] INAF, Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50125 Florence, Italy
[44] Acad Sinica, Inst Astron & Astrophys, 1,Sect 4,Roosevelt Rd, Taipei 10617, Taiwan
[45] European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany
[46] Univ Autanoma Madrid, Fac Ciencias, Dept Fis Teor, Modulo 8, Madrid 28049, Spain
[47] Univ Autanoma Madrid, Fac Ciencias, CIAFF, Modulo 8, Madrid 28049, Spain
[48] Univ Atacama, Inst Astron & Ciencias Planetarias Atacama INCT, Copayapu 485, Copiapo, Chile
[49] Univ Padua, Dipartimento Fis & Astron G Galilei, Vicolo Osservatorio 3, I-35122 Padua, Italy
[50] INAF, Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35122 Padua, Italy
基金
欧盟地平线“2020”; 欧洲研究理事会; 英国科学技术设施理事会;
关键词
galaxies: clusters: general; galaxies: clusters: intracluster medium; large-scale structure of Universe; dark matter; cosmology: observations; ZELDOVICH EFFECT OBSERVATIONS; ATACAMA COSMOLOGY TELESCOPE; NONTHERMAL PRESSURE SUPPORT; WEAK-LENSING SHEAR; COOL-CORE CLUSTERS; 2 GALAXY CLUSTERS; SZ LARGE PROGRAM; X-RAY; INTRACLUSTER MEDIUM; JOINT ANALYSIS;
D O I
10.1051/0004-6361/202039632
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Cluster HEritage project with XMM-Newton - Mass Assembly and Thermodynamics at the Endpoint of structure formation (CHEX-MATE) is a three-mega-second Multi-Year Heritage Programme to obtain X-ray observations of a minimally-biased, signal-to-noise-limited sample of 118 galaxy clusters detected by Planck through the Sunyaev-Zeldovich effect. The programme, described in detail in this paper, aims to study the ultimate products of structure formation in time and mass. It is composed of a census of the most recent objects to have formed (Tier-1: 0.05<z<0.2; 2x10(14) M-circle dot<M-500<9x10(14) M-<circle dot>), together with a sample of the highest mass objects in the Universe (Tier-2: z<0.6; M-500>7.25x10(14) M-<circle dot>). The programme will yield an accurate vision of the statistical properties of the underlying population, measure how the gas properties are shaped by collapse into the dark matter halo, uncover the provenance of non-gravitational heating, and resolve the major uncertainties in mass determination that limit the use of clusters for cosmological parameter estimation. We will acquire X-ray exposures of uniform depth, designed to obtain individual mass measurements accurate to 15-20% under the hydrostatic assumption. We present the project motivations, describe the programme definition, and detail the ongoing multi-wavelength observational (lensing, SZ, radio) and theoretical effort that is being deployed in support of the project.
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