papers

Publications (23)

astro-ph.CO2011

Planck Early Results. X. Statistical analysis of Sunyaev-Zeldovich scaling relations for X-ray galaxy clusters

Planck Collaboration, N. Aghanim, M. Arnaud +197

All-sky data from the Planck survey and the Meta-Catalogue of X-ray detected Clusters of galaxies (MCXC) are combined to investigate the relationship between the thermal Sunyaev-Ze…

astro-ph.CO2012

Planck intermediate results. VIII. Filaments between interacting clusters

Planck Collaboration, P. A. R. Ade, N. Aghanim +208

About half of the baryons of the Universe are expected to be in the form of filaments of hot and low density intergalactic medium. Most of these baryons remain undetected even by t…

astro-ph.CO2009

The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the Y_SZ-M_500 relation

M. Arnaud, G. W. Pratt, R. Piffaretti +3

(abridged) We investigate the regularity of cluster pressure profiles with REXCESS, a representative sample of 33 local clusters observed with XMM-Newton. The sample spans a mass r…

astro-ph2003

Spatially resolved X-ray spectroscopy of cooling clusters of galaxies

J. S. Kaastra, T. Tamura, J. R. Peterson +7

We present spatially resolved X-ray spectra taken with the EPIC cameras of XMM-Newton of a sample of 17 cooling clusters and three non-cooling clusters for comparison. The deprojec…

astro-ph.CO2012

Planck intermediate results. VI: The dynamical structure of PLCKG214.6+37.0, a Planck discovered triple system of galaxy clusters

Planck Collaboration, P. A. R. Ade, N. Aghanim +200

The survey of galaxy clusters performed by Planck through the Sunyaev-Zeldovich effect has already discovered many interesting objects, thanks to the whole coverage of the sky. One…

astro-ph.CO2012

Planck intermediate results. III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal

Planck Collaboration, P. A. R. Ade, N. Aghanim +183

We examine the relation between the galaxy cluster mass M and Sunyaev-Zeldovich (SZ) effect signal D_A^2 Y for a sample of 19 objects for which weak lensing (WL) mass measurements…

astro-ph.CO2011

Planck Early Results XI: Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations

Planck Collaboration, P. A. R. Ade, N. Aghanim +207

We present precise Sunyaev-Zeldovich (SZ) effect measurements in the direction of 62 nearby galaxy clusters (z <0.5) detected at high signal-to-noise in the first Planck all-sky da…

astro-ph2000

Shape and geometry of galaxy clusters and the SZ effect

L. Grenacher, R. Piffaretti, D. Puy +2

We discuss the influence of the finite extension and the geometry of clusters of galaxies, as well as of the polytropic temperature profile, on the determination of the Hubble cons…

astro-ph.CO2010

The galaxy cluster Ysz-Lx and Ysz-M relations from the WMAP 5-yr data

J. -B. Melin, J. G. Bartlett, J. Delabrouille +3

We use multifrequency matched filters to estimate, in the WMAP 5-year data, the Sunyaev-Zel'dovich (SZ) fluxes of 893 ROSAT NORAS/REFLEX clusters spanning the luminosity range Lx,[…

astro-ph.CO2012

Planck Intermediate Results. XI: The gas content of dark matter halos: the Sunyaev-Zeldovich-stellar mass relation for locally brightest galaxies

Planck Collaboration, P. A. R. Ade, N. Aghanim +194

We present the scaling relation between Sunyaev-Zeldovich (SZ) signal and stellar mass for almost 260,000 locally brightest galaxies (LBGs) selected from the Sloan Digital Sky Surv…

astro-ph.CO2011

Planck Early Results XXVI: Detection with Planck and confirmation by XMM-Newton of PLCK G266.6-27.3, an exceptionally X-ray luminous and massive galaxy cluster at z~1

Planck Collaboration, N. Aghanim, M. Arnaud +189

We present first results on PLCK G266.6-27.3, a galaxy cluster candidate detected at a signal-to-noise ratio of 5 in the Planck All Sky survey. An XMM-Newton validation observation…

astro-ph.CO2010

The MCXC: a Meta-Catalogue of X-ray detected Clusters of galaxies

R. Piffaretti, M. Arnaud, G. W. Pratt +2

We present the compilation and properties of a Meta-Catalogue of X-ray detected Clusters of galaxies, the MCXC. This very large catalogue is based on publicly available ROSAT All S…

astro-ph2002

Morphology of Galaxy Clusters and Sunyaev-Zel'dovich effect

Ph. Jetzer, P. Koch, R. Piffaretti +2

Observations of the X-ray band wavelength reveal an evident ellipticity of many galaxy clusters atmospheres. The modeling of the intracluster gas with an ellipsoidal -model lea…

astro-ph.CO2012

Planck intermediate results. X. Physics of the hot gas in the Coma cluster

Planck Collaboration, P. A. R. Ade, N. Aghanim +207

We present an analysis of Planck satellite data on the Coma Cluster observed via the Sunyaev-Zeldovich effect. Planck is able, for the first time, to detect SZ emission up to r ~ 3…

astro-ph2001

Sunyaev-Zel'dovich Effect and Morphology of Galaxy Clusters

R. Piffaretti, Ph. Jetzer, D. Puy +1

We investigate the influence of the finite extension and the aspherical geometry of a galaxy cluster on the estimate of the Hubble constant through the Sunyaev-Zel'dovich effect. A…

astro-ph.CO2011

Planck early results: Cluster Sunyaev-Zeldovich optical scaling relations

Planck Collaboration, N. Aghanim, M. Arnaud +202

We present the Sunyaev-Zeldovich (SZ) signal-to-richness scaling relation (Y500-N200) for the MaxBCG cluster catalogue. Employing a multi-frequency matched filter on the Planck sky…

astro-ph.CO2012

Planck Intermediate Results. IV. The XMM-Newton validation programme for new Planck galaxy clusters

Planck Collaboration, P. A. R. Ade, N. Aghanim +191

We present the final results from the XMM-Newton validation follow-up of new Planck galaxy cluster candidates. We observed 15 new candidates, detected with signal-to-noise ratios b…

astro-ph.CO2011

Planck Early Results VIII: The all-sky Early Sunyaev-Zeldovich cluster sample

Planck Collaboration, P. A. R. Ade, N. Aghanim +235

We present the first all-sky sample of galaxy clusters detected blindly by the Planck satellite through the Sunyaev-Zeldovich (SZ) effect from its six highest frequencies. This ear…

astro-ph.CO2012

The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths

J. Delabrouille, M. Betoule, J. -B. Melin +39

We present the Planck Sky Model (PSM), a parametric model for the generation of all-sky, few arcminute resolution maps of sky emission at submillimetre to centimetre wavelengths, i…

astro-ph.CO2012

Planck Intermediate Results. V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect

Planck Collaboration, P. A. R. Ade, N. Aghanim +214

Taking advantage of the all-sky coverage and broad frequency range of the Planck satellite, we study the Sunyaev-Zeldovich (SZ) and pressure profiles of 62 nearby massive clusters…

astro-ph.CO2011

Planck Early Results. VII. The Early Release Compact Source Catalog

Planck Collaboration, P. A. R. Ade, N. Aghanim +228

(Abridged) A brief description of the methodology of construction, contents and usage of the Planck Early Release Compact Source Catalogue (ERCSC), including the Early Cold Cores (…

astro-ph.CO2009

Gas entropy in a representative sample of nearby X-ray galaxy clusters (REXCESS): relationship to gas mass fraction

G. W. Pratt, M. Arnaud, R. Piffaretti +6

(Abridged) We examine the radial entropy distribution and its scaling using 31 nearby galaxy clusters from the Representative XMM-Newton Cluster Structure Survey (REXCESS). The ent…

astro-ph.CO2011

Planck early results. IX. XMM-Newton follow-up for validation of Planck cluster candidates

Planck Collaboration, N. Aghanim, M. Arnaud +197

We present the XMM-Newton follow-up for confirmation of Planck cluster candidates. Twenty-five candidates have been observed to date using snapshot (~10 ksec) exposures, ten as par…