@article{10902/28458,
year = {2011},
month = {12},
url = {https://hdl.handle.net/10902/28458},
abstract = {We present precise Sunyaev-Zeldovich (SZ) effect measurements in the direction of 62 nearby galaxy clusters (z < 0.5) detected at high signal-tonoise in the first Planck all-sky data set. The sample spans approximately a decade in total mass, 2 × 1014 M < M500 < 2 × 1015 M, where M500 is the mass corresponding to a total density contrast of 500. Combining these high quality Planck measurements with deep XMM-Newton X-ray
data, we investigate the relations between D2 A Y500, the integrated Compton parameter due to the SZ effect, and the X-ray-derived gas mass Mg,500, temperature TX, luminosity LX,500, SZ signal analogue YX,500 = Mg,500 × TX, and total mass M500. After correction for the effect of selection bias on the scaling relations, we find results that are in excellent agreement with both X-ray predictions and recently-published ground-based data derived from smaller samples. The present data yield an exceptionally robust, high-quality local reference, and illustrate Planck?s unique capabilities for all-sky statistical studies of galaxy clusters.},
organization = {The Planck Collaboration acknowledges the support of: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN and JA (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and DEISA (EU). The present work is partly based on observations obtained with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and the USA (NASA). This research has made use of the following databases: SIMBAD, operated at CDS, Strasbourg, France; the NED database, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space
Administration; BAX, which is operated by the Laboratoire d’Astrophysique de Tarbes-Toulouse (LATT), under contract with the Centre National d’Etudes Spatiales (CNES). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.rssd.esa.int/Planck.},
publisher = {EDP Sciences},
publisher = {Astronomy and Astrophysics, 2011, 536, A11},
title = {Planck early results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations},
author = {Ade, Peter Anthony Robert and Aghanim, Nabila and Arnaud, M. and Ashdown, Mark and Aumont, J. and Baccigalupi, C. and Balbi, A. and Banday, A. J. and Barreiro Vilas, Rita Belén and Bartelmann, M. and Bartlett, J. G. and Battaner, E. and Benabed, K. and Benoît, A. and Bernard, J.-P. and Diego Rodríguez, José María and Herranz Muñoz, Diego and López-Caniego Alcarria, Marcos and Martínez González, Enrique and Vielva Martínez, Patricio},
}