Final published version
Research output: Contribution to Journal/Magazine › Journal article › peer-review
Research output: Contribution to Journal/Magazine › Journal article › peer-review
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TY - JOUR
T1 - The XMM Cluster Survey
T2 - Predicted overlap with the Planck Cluster Catalogue
AU - Viana, Pedro T. P.
AU - Da Silva, António
AU - Ramos, Elsa P. R. G.
AU - Liddle, Andrew R.
AU - Lloyd-Davies, E. J.
AU - Romer, A. Kathy
AU - Kay, Scott T.
AU - Collins, Chris A.
AU - Hilton, Matt
AU - Hosmer, Mark
AU - Hoyle, Ben
AU - Mayers, Julian A.
AU - Mehrtens, Nicola
AU - Miller, Christopher J.
AU - Sahlén, Martin
AU - Stanford, S. Adam
AU - Stott, John P.
PY - 2012/5/11
Y1 - 2012/5/11
N2 - We present a list of 15 clusters of galaxies, serendipitously detected by the XMM Cluster Survey (XCS), that have a high probability of detection by the Planck satellite. Three of them already appear in the Planck Early Sunyaev-Zel'dovich (ESZ) catalogue. The estimation of the Planck detection probability assumes the flat Lambda cold dark matter (ΛCDM) cosmology most compatible with 7-year Wilkinson Microwave Anisotropy Probe (WMAP7) data. It takes into account the XCS selection function and Planck sensitivity, as well as the covariance of the cluster X-ray luminosity, temperature and integrated Comptonization parameter, as a function of cluster mass and redshift, determined by the Millennium gas simulations. We also characterize the properties of the galaxy clusters in the final data release of the XCS that we expect Planck will have detected by the end of its extended mission. Finally, we briefly discuss possible joint applications of the XCS and Planck data.
AB - We present a list of 15 clusters of galaxies, serendipitously detected by the XMM Cluster Survey (XCS), that have a high probability of detection by the Planck satellite. Three of them already appear in the Planck Early Sunyaev-Zel'dovich (ESZ) catalogue. The estimation of the Planck detection probability assumes the flat Lambda cold dark matter (ΛCDM) cosmology most compatible with 7-year Wilkinson Microwave Anisotropy Probe (WMAP7) data. It takes into account the XCS selection function and Planck sensitivity, as well as the covariance of the cluster X-ray luminosity, temperature and integrated Comptonization parameter, as a function of cluster mass and redshift, determined by the Millennium gas simulations. We also characterize the properties of the galaxy clusters in the final data release of the XCS that we expect Planck will have detected by the end of its extended mission. Finally, we briefly discuss possible joint applications of the XCS and Planck data.
KW - Galaxies: clusters: general
U2 - 10.1111/j.1365-2966.2012.20673.x
DO - 10.1111/j.1365-2966.2012.20673.x
M3 - Journal article
AN - SCOPUS:84863404158
VL - 422
SP - 1007
EP - 1013
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
SN - 0035-8711
IS - 2
ER -