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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Veröffentlicht in:Astronomy and astrophysics (Berlin) 2017, Vol.597, p.A110
Hauptverfasser: 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.
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container_title Astronomy and astrophysics (Berlin)
container_volume 597
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. 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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. 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Here we illustrate an application of high resolution (&lt;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. 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recordid cdi_hal_primary_oai_HAL_in2p3_01349507v1
source Bacon EDP Sciences France Licence nationale-ISTEX-PS-Journals-PFISTEX; EDP Sciences; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals
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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