Non-parametric deprojection of NIKA SZ observations: Pressure distribution in the Planck-discovered cluster PSZ1 G045.85+57.71
The determination of the thermodynamic properties of clusters of galaxies at intermediate and high redshift can bring new insights into the formation of large-scale structures. It is essential for a robust calibration of the mass-observable scaling relations and their scatter, which are key ingredie...
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creator | Ruppin, F. Adam, R. Comis, B. Ade, P. André, P. Arnaud, M. Beelen, A. Benoît, A. Bideaud, A. Billot, N. Bourrion, O. Calvo, M. Catalano, A. Coiffard, G. D’Addabbo, A. De Petris, M. Désert, F.-X. Doyle, S. Goupy, J. Kramer, C. Leclercq, S. Macías-Pérez, J. F. Mauskopf, P. Mayet, F. Monfardini, A. Pajot, F. Pascale, E. Perotto, L. Pisano, G. Pointecouteau, E. Ponthieu, N. Pratt, G. W. Revéret, V. Ritacco, A. Rodriguez, L. Romero, C. Schuster, K. Sievers, A. Triqueneaux, S. Tucker, C. Zylka, R. |
description | The determination of the thermodynamic properties of clusters of galaxies at intermediate and high redshift can bring new insights into the formation of large-scale structures. It is essential for a robust calibration of the mass-observable scaling relations and their scatter, which are key ingredients for precise cosmology using cluster statistics. Here we illustrate an application of high resolution ( |
doi_str_mv | 10.1051/0004-6361/201629405 |
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F. ; Mauskopf, P. ; Mayet, F. ; Monfardini, A. ; Pajot, F. ; Pascale, E. ; Perotto, L. ; Pisano, G. ; Pointecouteau, E. ; Ponthieu, N. ; Pratt, G. W. ; Revéret, V. ; Ritacco, A. ; Rodriguez, L. ; Romero, C. ; Schuster, K. ; Sievers, A. ; Triqueneaux, S. ; Tucker, C. ; Zylka, R.</creator><creatorcontrib>Ruppin, F. ; Adam, R. ; Comis, B. ; Ade, P. ; André, P. ; Arnaud, M. ; Beelen, A. ; Benoît, A. ; Bideaud, A. ; Billot, N. ; Bourrion, O. ; Calvo, M. ; Catalano, A. ; Coiffard, G. ; D’Addabbo, A. ; De Petris, M. ; Désert, F.-X. ; Doyle, S. ; Goupy, J. ; Kramer, C. ; Leclercq, S. ; Macías-Pérez, J. F. ; Mauskopf, P. ; Mayet, F. ; Monfardini, A. ; Pajot, F. ; Pascale, E. ; Perotto, L. ; Pisano, G. ; Pointecouteau, E. ; Ponthieu, N. ; Pratt, G. W. ; Revéret, V. ; Ritacco, A. ; Rodriguez, L. ; Romero, C. ; Schuster, K. ; Sievers, A. ; Triqueneaux, S. ; Tucker, C. ; Zylka, R.</creatorcontrib><description>The determination of the thermodynamic properties of clusters of galaxies at intermediate and high redshift can bring new insights into the formation of large-scale structures. It is essential for a robust calibration of the mass-observable scaling relations and their scatter, which are key ingredients for precise cosmology using cluster statistics. Here we illustrate an application of high resolution (<20 arcsec) thermal Sunyaev-Zel’dovich (tSZ) observations by probing the intracluster medium (ICM) of the Planck-discovered galaxy cluster PSZ1 G045.85+57.71 at redshift z = 0.61, using tSZ data obtained with the NIKA camera, which is a dual-band (150 and 260 GHz) instrument operated at the IRAM 30-m telescope. We deproject jointly NIKA and Planck data to extract the electronic pressure distribution from the cluster core (R ~ 0.02 R500) to its outskirts (R ~ 3 R500) non-parametrically for the first time at intermediate redshift. The constraints on the resulting pressure profile allow us to reduce the relative uncertainty on the integrated Compton parameter by a factor of two compared to the Planck value. Combining the tSZ data and the deprojected electronic density profile from XMM-Newton allows us to undertake a hydrostatic mass analysis, for which we study the impact of a spherical model assumption on the total mass estimate. We also investigate the radial temperature and entropy distributions. These data indicate that PSZ1 G045.85+57.71 is a massive (M500 ~ 5.5 × 1014M⊙) cool-core cluster. This work is part of a pilot study aiming at optimizing the treatment of the NIKA2 tSZ large program dedicated to the follow-up of SZ-discovered clusters at intermediate and high redshifts. 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W.</creatorcontrib><creatorcontrib>Revéret, V.</creatorcontrib><creatorcontrib>Ritacco, A.</creatorcontrib><creatorcontrib>Rodriguez, L.</creatorcontrib><creatorcontrib>Romero, C.</creatorcontrib><creatorcontrib>Schuster, K.</creatorcontrib><creatorcontrib>Sievers, A.</creatorcontrib><creatorcontrib>Triqueneaux, S.</creatorcontrib><creatorcontrib>Tucker, C.</creatorcontrib><creatorcontrib>Zylka, R.</creatorcontrib><title>Non-parametric deprojection of NIKA SZ observations: Pressure distribution in the Planck-discovered cluster PSZ1 G045.85+57.71</title><title>Astronomy and astrophysics (Berlin)</title><description>The determination of the thermodynamic properties of clusters of galaxies at intermediate and high redshift can bring new insights into the formation of large-scale structures. It is essential for a robust calibration of the mass-observable scaling relations and their scatter, which are key ingredients for precise cosmology using cluster statistics. Here we illustrate an application of high resolution (<20 arcsec) thermal Sunyaev-Zel’dovich (tSZ) observations by probing the intracluster medium (ICM) of the Planck-discovered galaxy cluster PSZ1 G045.85+57.71 at redshift z = 0.61, using tSZ data obtained with the NIKA camera, which is a dual-band (150 and 260 GHz) instrument operated at the IRAM 30-m telescope. We deproject jointly NIKA and Planck data to extract the electronic pressure distribution from the cluster core (R ~ 0.02 R500) to its outskirts (R ~ 3 R500) non-parametrically for the first time at intermediate redshift. The constraints on the resulting pressure profile allow us to reduce the relative uncertainty on the integrated Compton parameter by a factor of two compared to the Planck value. Combining the tSZ data and the deprojected electronic density profile from XMM-Newton allows us to undertake a hydrostatic mass analysis, for which we study the impact of a spherical model assumption on the total mass estimate. We also investigate the radial temperature and entropy distributions. These data indicate that PSZ1 G045.85+57.71 is a massive (M500 ~ 5.5 × 1014M⊙) cool-core cluster. This work is part of a pilot study aiming at optimizing the treatment of the NIKA2 tSZ large program dedicated to the follow-up of SZ-discovered clusters at intermediate and high redshifts. This study illustrates the potential of NIKA2 to put constraints on thethermodynamic properties and tSZ-scaling relations of these clusters, and demonstrates the excellent synergy between tSZ and X-ray observations of similar angular resolution.</description><subject>Astrophysics</subject><subject>cosmology: observations</subject><subject>galaxies: clusters: intracluster medium</subject><subject>instrumentation: high angular resolution</subject><subject>Physics</subject><issn>0004-6361</issn><issn>1432-0746</issn><issn>1432-0756</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><recordid>eNo9kMtOwkAUQCdGE_HxBW5mb4p3Xm1xR4giQpAEjYbNZDq9E6vQNjOF6M6tv-mXWMSwmty559zFIeSCQZeBYlcAIKNYxOyKA4t5T4I6IB0mBY8gkfEh6eyJY3ISwls7cpaKDvmaVmVUG29W2PjC0hxrX72hbYqqpJWj09G4T-cLWmUB_cZsv8M1nXkMYe2R5kVotWz9hxclbV6RzpamtO9Ru7LVBj3m1C7XoUFPZ_MF-_n6HoJU3VRdqqSbsDNy5Mwy4Pn_e0qebm8eB3fR5GE4GvQnkRVcNJFDY1IrlZJpbFPVM4AJIHdSAc-UwzxjHDkHwQ0ymSmGLnWsJ1MVi9waJ07J5e7uq1nq2hcr4z91ZQp915_oouS10MCE7ClINqylxY62vgrBo9srDPQ2ud4G1dugep-8taKd1VbBj71i_LuOE5EoncKzHg_5C5_dc70Qv-h-goQ</recordid><startdate>2017</startdate><enddate>2017</enddate><creator>Ruppin, F.</creator><creator>Adam, R.</creator><creator>Comis, B.</creator><creator>Ade, P.</creator><creator>André, P.</creator><creator>Arnaud, M.</creator><creator>Beelen, A.</creator><creator>Benoît, A.</creator><creator>Bideaud, A.</creator><creator>Billot, N.</creator><creator>Bourrion, O.</creator><creator>Calvo, M.</creator><creator>Catalano, A.</creator><creator>Coiffard, G.</creator><creator>D’Addabbo, A.</creator><creator>De Petris, M.</creator><creator>Désert, F.-X.</creator><creator>Doyle, S.</creator><creator>Goupy, J.</creator><creator>Kramer, C.</creator><creator>Leclercq, S.</creator><creator>Macías-Pérez, J. 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W.</au><au>Revéret, V.</au><au>Ritacco, A.</au><au>Rodriguez, L.</au><au>Romero, C.</au><au>Schuster, K.</au><au>Sievers, A.</au><au>Triqueneaux, S.</au><au>Tucker, C.</au><au>Zylka, R.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Non-parametric deprojection of NIKA SZ observations: Pressure distribution in the Planck-discovered cluster PSZ1 G045.85+57.71</atitle><jtitle>Astronomy and astrophysics (Berlin)</jtitle><date>2017</date><risdate>2017</risdate><volume>597</volume><spage>A110</spage><pages>A110-</pages><issn>0004-6361</issn><eissn>1432-0746</eissn><eissn>1432-0756</eissn><abstract>The determination of the thermodynamic properties of clusters of galaxies at intermediate and high redshift can bring new insights into the formation of large-scale structures. It is essential for a robust calibration of the mass-observable scaling relations and their scatter, which are key ingredients for precise cosmology using cluster statistics. Here we illustrate an application of high resolution (<20 arcsec) thermal Sunyaev-Zel’dovich (tSZ) observations by probing the intracluster medium (ICM) of the Planck-discovered galaxy cluster PSZ1 G045.85+57.71 at redshift z = 0.61, using tSZ data obtained with the NIKA camera, which is a dual-band (150 and 260 GHz) instrument operated at the IRAM 30-m telescope. We deproject jointly NIKA and Planck data to extract the electronic pressure distribution from the cluster core (R ~ 0.02 R500) to its outskirts (R ~ 3 R500) non-parametrically for the first time at intermediate redshift. The constraints on the resulting pressure profile allow us to reduce the relative uncertainty on the integrated Compton parameter by a factor of two compared to the Planck value. Combining the tSZ data and the deprojected electronic density profile from XMM-Newton allows us to undertake a hydrostatic mass analysis, for which we study the impact of a spherical model assumption on the total mass estimate. We also investigate the radial temperature and entropy distributions. These data indicate that PSZ1 G045.85+57.71 is a massive (M500 ~ 5.5 × 1014M⊙) cool-core cluster. This work is part of a pilot study aiming at optimizing the treatment of the NIKA2 tSZ large program dedicated to the follow-up of SZ-discovered clusters at intermediate and high redshifts. This study illustrates the potential of NIKA2 to put constraints on thethermodynamic properties and tSZ-scaling relations of these clusters, and demonstrates the excellent synergy between tSZ and X-ray observations of similar angular resolution.</abstract><pub>EDP Sciences</pub><doi>10.1051/0004-6361/201629405</doi><orcidid>https://orcid.org/0000-0003-3201-0185</orcidid><orcidid>https://orcid.org/0009-0009-2877-2954</orcidid><orcidid>https://orcid.org/0000-0001-9995-4792</orcidid><orcidid>https://orcid.org/0000-0001-6937-5052</orcidid><orcidid>https://orcid.org/0000-0001-8488-3645</orcidid><orcidid>https://orcid.org/0009-0000-5380-1109</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Astrophysics cosmology: observations galaxies: clusters: intracluster medium instrumentation: high angular resolution Physics |
title | Non-parametric deprojection of NIKA SZ observations: Pressure distribution in the Planck-discovered cluster PSZ1 G045.85+57.71 |
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