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.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics cosmology: observations galaxies: clusters: intracluster medium instrumentation: high angular resolution Physics
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Beschreibung
Zusammenfassung:	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 (
ISSN:	0004-6361 1432-0746 1432-0756
DOI:	10.1051/0004-6361/201629405