The Cluster HEritage project with XMM-Newton : Mass Assembly and Thermodynamics at the Endpoint of structure formation: I. Programme overview
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 b...
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| Veröffentlicht in: | Astronomy and astrophysics (Berlin) 2021-06, Vol.650, p.A104 |
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| creator | Arnaud, M. Ettori, S. Pratt, G. W. Rossetti, M. Eckert, D. Gastaldello, F. Gavazzi, R. Kay, S.T. Lovisari, L. Maughan, B.J. Pointecouteau, E. Sereno, M. Bartalucci, I. Bonafede, A. Bourdin, H. Cassano, R. Duffy, R.T. Iqbal, A. Maurogordato, S. Rasia, E. Sayers, J. Andrade-Santos, F. Aussel, H. Barnes, D.J. Barrena, R. Borgani, S. Burkutean, S. Clerc, N. Corasaniti, P.-S. Cuillandre, J.-C. De Grandi, S. De Petris, M. Dolag, K. Donahue, M. Ferragamo, A. Gaspari, M. Ghizzardi, S. Gitti, M. Haines, C.P. Jauzac, M. Johnston-Hollitt, M. Jones, C. Kéruzoré, F. LeBrun, A.M.C. Mayet, F. Mazzotta, P. Melin, J.-B. Molendi, S. Nonino, M. Okabe, N. Paltani, S. Perotto, L. Pires, S. Radovich, M. Rubino-Martin, J.-A. Salvati, L. Saro, A. Sartoris, B. Schellenberger, G. Streblyanska, A. Tarrío, P. Tozzi, P. Umetsu, K. van der Burg, R.F.J. Vazza, F. Venturi, T. Yepes, G. Zarattini, S. |
| description | 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 |
| doi_str_mv | 10.1051/0004-6361/202039632 |
| format | Article |
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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; 2 × 10
14
M
⊙
<
M
500
< 9 × 10
14
M
⊙
), together with a sample of the highest mass objects in the Universe (Tier-2:
z
< 0.6;
M
500
> 7.25 × 10
14
M
⊙
). 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.</description><identifier>ISSN: 0004-6361</identifier><identifier>EISSN: 1432-0746</identifier><identifier>EISSN: 1432-0756</identifier><identifier>DOI: 10.1051/0004-6361/202039632</identifier><language>eng</language><publisher>EDP Sciences</publisher><subject>Astrophysics ; Cosmology and Extra-Galactic Astrophysics ; Physics</subject><ispartof>Astronomy and astrophysics (Berlin), 2021-06, Vol.650, p.A104</ispartof><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c233t-7ad8bb0785ea8e2bbddcc88c39e64af476479182943931c22565a53536c85b523</cites><orcidid>0000-0001-6342-9662 ; 0000-0002-5477-8454 ; 0000-0003-4046-0637 ; 0000-0002-9288-862X ; 0000-0002-0296-1011 ; 0000-0002-9605-5588 ; 0000-0001-6937-5052 ; 0000-0002-1371-5705 ; 0000-0001-9995-4792 ; 0000-0002-8108-9179 ; 0000-0002-5540-6935 ; 0000-0001-8488-3645 ; 0000-0002-5068-4581</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,776,780,881,3713,27903,27904</link.rule.ids><backlink>$$Uhttps://hal.science/hal-02991777$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Arnaud, M.</creatorcontrib><creatorcontrib>Ettori, S.</creatorcontrib><creatorcontrib>Pratt, G. W.</creatorcontrib><creatorcontrib>Rossetti, M.</creatorcontrib><creatorcontrib>Eckert, D.</creatorcontrib><creatorcontrib>Gastaldello, F.</creatorcontrib><creatorcontrib>Gavazzi, R.</creatorcontrib><creatorcontrib>Kay, S.T.</creatorcontrib><creatorcontrib>Lovisari, L.</creatorcontrib><creatorcontrib>Maughan, B.J.</creatorcontrib><creatorcontrib>Pointecouteau, E.</creatorcontrib><creatorcontrib>Sereno, M.</creatorcontrib><creatorcontrib>Bartalucci, I.</creatorcontrib><creatorcontrib>Bonafede, A.</creatorcontrib><creatorcontrib>Bourdin, H.</creatorcontrib><creatorcontrib>Cassano, R.</creatorcontrib><creatorcontrib>Duffy, R.T.</creatorcontrib><creatorcontrib>Iqbal, A.</creatorcontrib><creatorcontrib>Maurogordato, S.</creatorcontrib><creatorcontrib>Rasia, E.</creatorcontrib><creatorcontrib>Sayers, J.</creatorcontrib><creatorcontrib>Andrade-Santos, F.</creatorcontrib><creatorcontrib>Aussel, H.</creatorcontrib><creatorcontrib>Barnes, D.J.</creatorcontrib><creatorcontrib>Barrena, R.</creatorcontrib><creatorcontrib>Borgani, S.</creatorcontrib><creatorcontrib>Burkutean, S.</creatorcontrib><creatorcontrib>Clerc, N.</creatorcontrib><creatorcontrib>Corasaniti, P.-S.</creatorcontrib><creatorcontrib>Cuillandre, J.-C.</creatorcontrib><creatorcontrib>De Grandi, S.</creatorcontrib><creatorcontrib>De Petris, M.</creatorcontrib><creatorcontrib>Dolag, K.</creatorcontrib><creatorcontrib>Donahue, M.</creatorcontrib><creatorcontrib>Ferragamo, A.</creatorcontrib><creatorcontrib>Gaspari, M.</creatorcontrib><creatorcontrib>Ghizzardi, S.</creatorcontrib><creatorcontrib>Gitti, M.</creatorcontrib><creatorcontrib>Haines, C.P.</creatorcontrib><creatorcontrib>Jauzac, M.</creatorcontrib><creatorcontrib>Johnston-Hollitt, M.</creatorcontrib><creatorcontrib>Jones, C.</creatorcontrib><creatorcontrib>Kéruzoré, F.</creatorcontrib><creatorcontrib>LeBrun, A.M.C.</creatorcontrib><creatorcontrib>Mayet, F.</creatorcontrib><creatorcontrib>Mazzotta, P.</creatorcontrib><creatorcontrib>Melin, J.-B.</creatorcontrib><creatorcontrib>Molendi, S.</creatorcontrib><creatorcontrib>Nonino, M.</creatorcontrib><creatorcontrib>Okabe, N.</creatorcontrib><creatorcontrib>Paltani, S.</creatorcontrib><creatorcontrib>Perotto, L.</creatorcontrib><creatorcontrib>Pires, S.</creatorcontrib><creatorcontrib>Radovich, M.</creatorcontrib><creatorcontrib>Rubino-Martin, J.-A.</creatorcontrib><creatorcontrib>Salvati, L.</creatorcontrib><creatorcontrib>Saro, A.</creatorcontrib><creatorcontrib>Sartoris, B.</creatorcontrib><creatorcontrib>Schellenberger, G.</creatorcontrib><creatorcontrib>Streblyanska, A.</creatorcontrib><creatorcontrib>Tarrío, P.</creatorcontrib><creatorcontrib>Tozzi, P.</creatorcontrib><creatorcontrib>Umetsu, K.</creatorcontrib><creatorcontrib>van der Burg, R.F.J.</creatorcontrib><creatorcontrib>Vazza, F.</creatorcontrib><creatorcontrib>Venturi, T.</creatorcontrib><creatorcontrib>Yepes, G.</creatorcontrib><creatorcontrib>Zarattini, S.</creatorcontrib><creatorcontrib>The CHEX-MATE Collaboration</creatorcontrib><title>The Cluster HEritage project with XMM-Newton : Mass Assembly and Thermodynamics at the Endpoint of structure formation: I. Programme overview</title><title>Astronomy and astrophysics (Berlin)</title><description>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; 2 × 10
14
M
⊙
<
M
500
< 9 × 10
14
M
⊙
), together with a sample of the highest mass objects in the Universe (Tier-2:
z
< 0.6;
M
500
> 7.25 × 10
14
M
⊙
). 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.</description><subject>Astrophysics</subject><subject>Cosmology and Extra-Galactic Astrophysics</subject><subject>Physics</subject><issn>0004-6361</issn><issn>1432-0746</issn><issn>1432-0756</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><recordid>eNo9kD1PwzAQQC0EEqXwC1huZQj1R_wRtqoqFKmFpUhsluM4NFUSV7Zb1H9Po6JOpzu9e8ND6JHgZ4I5mWCM80wwQSYUU8wKwegVGpGc0QzLXFyj0YW4RXcxbk8rJYqN0GG9cTBr9zG5AIt5aJL5cbALfutsgt8mbeB7tco-3G_yPbzAysQI0xhdV7ZHMH0FJ0HofHXsTdfYCCZBOinnfbXzTZ_A1xBT2Nu0Dw5qHzqTGt_fo5vatNE9_M8x-nqdr2eLbPn59j6bLjNLGUuZNJUqSywVd0Y5WpZVZa1SlhVO5KbOpchlQRQtclYwYinlghvOOBNW8ZJTNkZPZ-_GtHoXms6Eo_am0YvpUg83TIuCSCkPA8vOrA0-xuDqywPBesish4h6iKgvmdkf1sFvlw</recordid><startdate>20210601</startdate><enddate>20210601</enddate><creator>Arnaud, M.</creator><creator>Ettori, S.</creator><creator>Pratt, G. 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W. ; Rossetti, M. ; Eckert, D. ; Gastaldello, F. ; Gavazzi, R. ; Kay, S.T. ; Lovisari, L. ; Maughan, B.J. ; Pointecouteau, E. ; Sereno, M. ; Bartalucci, I. ; Bonafede, A. ; Bourdin, H. ; Cassano, R. ; Duffy, R.T. ; Iqbal, A. ; Maurogordato, S. ; Rasia, E. ; Sayers, J. ; Andrade-Santos, F. ; Aussel, H. ; Barnes, D.J. ; Barrena, R. ; Borgani, S. ; Burkutean, S. ; Clerc, N. ; Corasaniti, P.-S. ; Cuillandre, J.-C. ; De Grandi, S. ; De Petris, M. ; Dolag, K. ; Donahue, M. ; Ferragamo, A. ; Gaspari, M. ; Ghizzardi, S. ; Gitti, M. ; Haines, C.P. ; Jauzac, M. ; Johnston-Hollitt, M. ; Jones, C. ; Kéruzoré, F. ; LeBrun, A.M.C. ; Mayet, F. ; Mazzotta, P. ; Melin, J.-B. ; Molendi, S. ; Nonino, M. ; Okabe, N. ; Paltani, S. ; Perotto, L. ; Pires, S. ; Radovich, M. ; Rubino-Martin, J.-A. ; Salvati, L. ; Saro, A. ; Sartoris, B. ; Schellenberger, G. ; Streblyanska, A. ; Tarrío, P. ; Tozzi, P. ; Umetsu, K. ; van der Burg, R.F.J. ; Vazza, F. ; Venturi, T. ; Yepes, G. ; Zarattini, S.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c233t-7ad8bb0785ea8e2bbddcc88c39e64af476479182943931c22565a53536c85b523</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Astrophysics</topic><topic>Cosmology and Extra-Galactic Astrophysics</topic><topic>Physics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Arnaud, M.</creatorcontrib><creatorcontrib>Ettori, S.</creatorcontrib><creatorcontrib>Pratt, G. W.</creatorcontrib><creatorcontrib>Rossetti, M.</creatorcontrib><creatorcontrib>Eckert, D.</creatorcontrib><creatorcontrib>Gastaldello, F.</creatorcontrib><creatorcontrib>Gavazzi, R.</creatorcontrib><creatorcontrib>Kay, S.T.</creatorcontrib><creatorcontrib>Lovisari, L.</creatorcontrib><creatorcontrib>Maughan, B.J.</creatorcontrib><creatorcontrib>Pointecouteau, E.</creatorcontrib><creatorcontrib>Sereno, M.</creatorcontrib><creatorcontrib>Bartalucci, I.</creatorcontrib><creatorcontrib>Bonafede, A.</creatorcontrib><creatorcontrib>Bourdin, H.</creatorcontrib><creatorcontrib>Cassano, R.</creatorcontrib><creatorcontrib>Duffy, R.T.</creatorcontrib><creatorcontrib>Iqbal, A.</creatorcontrib><creatorcontrib>Maurogordato, S.</creatorcontrib><creatorcontrib>Rasia, E.</creatorcontrib><creatorcontrib>Sayers, J.</creatorcontrib><creatorcontrib>Andrade-Santos, F.</creatorcontrib><creatorcontrib>Aussel, H.</creatorcontrib><creatorcontrib>Barnes, D.J.</creatorcontrib><creatorcontrib>Barrena, R.</creatorcontrib><creatorcontrib>Borgani, S.</creatorcontrib><creatorcontrib>Burkutean, S.</creatorcontrib><creatorcontrib>Clerc, N.</creatorcontrib><creatorcontrib>Corasaniti, P.-S.</creatorcontrib><creatorcontrib>Cuillandre, J.-C.</creatorcontrib><creatorcontrib>De Grandi, S.</creatorcontrib><creatorcontrib>De Petris, M.</creatorcontrib><creatorcontrib>Dolag, K.</creatorcontrib><creatorcontrib>Donahue, M.</creatorcontrib><creatorcontrib>Ferragamo, A.</creatorcontrib><creatorcontrib>Gaspari, M.</creatorcontrib><creatorcontrib>Ghizzardi, S.</creatorcontrib><creatorcontrib>Gitti, M.</creatorcontrib><creatorcontrib>Haines, C.P.</creatorcontrib><creatorcontrib>Jauzac, M.</creatorcontrib><creatorcontrib>Johnston-Hollitt, M.</creatorcontrib><creatorcontrib>Jones, C.</creatorcontrib><creatorcontrib>Kéruzoré, F.</creatorcontrib><creatorcontrib>LeBrun, A.M.C.</creatorcontrib><creatorcontrib>Mayet, F.</creatorcontrib><creatorcontrib>Mazzotta, P.</creatorcontrib><creatorcontrib>Melin, J.-B.</creatorcontrib><creatorcontrib>Molendi, S.</creatorcontrib><creatorcontrib>Nonino, M.</creatorcontrib><creatorcontrib>Okabe, N.</creatorcontrib><creatorcontrib>Paltani, S.</creatorcontrib><creatorcontrib>Perotto, L.</creatorcontrib><creatorcontrib>Pires, S.</creatorcontrib><creatorcontrib>Radovich, M.</creatorcontrib><creatorcontrib>Rubino-Martin, J.-A.</creatorcontrib><creatorcontrib>Salvati, L.</creatorcontrib><creatorcontrib>Saro, A.</creatorcontrib><creatorcontrib>Sartoris, B.</creatorcontrib><creatorcontrib>Schellenberger, G.</creatorcontrib><creatorcontrib>Streblyanska, A.</creatorcontrib><creatorcontrib>Tarrío, P.</creatorcontrib><creatorcontrib>Tozzi, P.</creatorcontrib><creatorcontrib>Umetsu, K.</creatorcontrib><creatorcontrib>van der Burg, R.F.J.</creatorcontrib><creatorcontrib>Vazza, F.</creatorcontrib><creatorcontrib>Venturi, T.</creatorcontrib><creatorcontrib>Yepes, G.</creatorcontrib><creatorcontrib>Zarattini, S.</creatorcontrib><creatorcontrib>The CHEX-MATE Collaboration</creatorcontrib><collection>CrossRef</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>Hyper Article en Ligne (HAL) (Open Access)</collection><jtitle>Astronomy and astrophysics (Berlin)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Arnaud, M.</au><au>Ettori, S.</au><au>Pratt, G. W.</au><au>Rossetti, M.</au><au>Eckert, D.</au><au>Gastaldello, F.</au><au>Gavazzi, R.</au><au>Kay, S.T.</au><au>Lovisari, L.</au><au>Maughan, B.J.</au><au>Pointecouteau, E.</au><au>Sereno, M.</au><au>Bartalucci, I.</au><au>Bonafede, A.</au><au>Bourdin, H.</au><au>Cassano, R.</au><au>Duffy, R.T.</au><au>Iqbal, A.</au><au>Maurogordato, S.</au><au>Rasia, E.</au><au>Sayers, J.</au><au>Andrade-Santos, F.</au><au>Aussel, H.</au><au>Barnes, D.J.</au><au>Barrena, R.</au><au>Borgani, S.</au><au>Burkutean, S.</au><au>Clerc, N.</au><au>Corasaniti, P.-S.</au><au>Cuillandre, J.-C.</au><au>De Grandi, S.</au><au>De Petris, M.</au><au>Dolag, K.</au><au>Donahue, M.</au><au>Ferragamo, A.</au><au>Gaspari, M.</au><au>Ghizzardi, S.</au><au>Gitti, M.</au><au>Haines, C.P.</au><au>Jauzac, M.</au><au>Johnston-Hollitt, M.</au><au>Jones, C.</au><au>Kéruzoré, F.</au><au>LeBrun, A.M.C.</au><au>Mayet, F.</au><au>Mazzotta, P.</au><au>Melin, J.-B.</au><au>Molendi, S.</au><au>Nonino, M.</au><au>Okabe, N.</au><au>Paltani, S.</au><au>Perotto, L.</au><au>Pires, S.</au><au>Radovich, M.</au><au>Rubino-Martin, J.-A.</au><au>Salvati, L.</au><au>Saro, A.</au><au>Sartoris, B.</au><au>Schellenberger, G.</au><au>Streblyanska, A.</au><au>Tarrío, P.</au><au>Tozzi, P.</au><au>Umetsu, K.</au><au>van der Burg, R.F.J.</au><au>Vazza, F.</au><au>Venturi, T.</au><au>Yepes, G.</au><au>Zarattini, S.</au><aucorp>The CHEX-MATE Collaboration</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The Cluster HEritage project with XMM-Newton : Mass Assembly and Thermodynamics at the Endpoint of structure formation: I. Programme overview</atitle><jtitle>Astronomy and astrophysics (Berlin)</jtitle><date>2021-06-01</date><risdate>2021</risdate><volume>650</volume><spage>A104</spage><pages>A104-</pages><issn>0004-6361</issn><eissn>1432-0746</eissn><eissn>1432-0756</eissn><abstract>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; 2 × 10
14
M
⊙
<
M
500
< 9 × 10
14
M
⊙
), together with a sample of the highest mass objects in the Universe (Tier-2:
z
< 0.6;
M
500
> 7.25 × 10
14
M
⊙
). 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.</abstract><pub>EDP Sciences</pub><doi>10.1051/0004-6361/202039632</doi><orcidid>https://orcid.org/0000-0001-6342-9662</orcidid><orcidid>https://orcid.org/0000-0002-5477-8454</orcidid><orcidid>https://orcid.org/0000-0003-4046-0637</orcidid><orcidid>https://orcid.org/0000-0002-9288-862X</orcidid><orcidid>https://orcid.org/0000-0002-0296-1011</orcidid><orcidid>https://orcid.org/0000-0002-9605-5588</orcidid><orcidid>https://orcid.org/0000-0001-6937-5052</orcidid><orcidid>https://orcid.org/0000-0002-1371-5705</orcidid><orcidid>https://orcid.org/0000-0001-9995-4792</orcidid><orcidid>https://orcid.org/0000-0002-8108-9179</orcidid><orcidid>https://orcid.org/0000-0002-5540-6935</orcidid><orcidid>https://orcid.org/0000-0001-8488-3645</orcidid><orcidid>https://orcid.org/0000-0002-5068-4581</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0004-6361 |
| ispartof | Astronomy and astrophysics (Berlin), 2021-06, Vol.650, p.A104 |
| issn | 0004-6361 1432-0746 1432-0756 |
| language | eng |
| recordid | cdi_hal_primary_oai_HAL_hal_02991777v2 |
| source | Bacon EDP Sciences France Licence nationale-ISTEX-PS-Journals-PFISTEX; EDP Sciences; EZB-FREE-00999 freely available EZB journals |
| subjects | Astrophysics Cosmology and Extra-Galactic Astrophysics Physics |
| title | The Cluster HEritage project with XMM-Newton : Mass Assembly and Thermodynamics at the Endpoint of structure formation: I. Programme overview |
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