The XMM Cluster Survey: predicted overlap with the Planck Cluster Catalogue

• Tipo: Artigo em Revista Científica Internacional
• Data: 2012

Autores

viana, ptp (Autor) FCUP; da silva, a (Autor) FCUP; ramos, eprg (Autor) Outra; liddle, ar (Autor) Outra; lloyd-davies, ej (Autor) Outra; romer, ak (Autor) Outra; kay, st (Autor) Outra; collins, ca (Autor) Outra; hilton, m (Autor) Outra; hosmer, m (Autor) Outra; hoyle, b (Autor) Outra; mayers, ja (Autor) Outra; mehrtens, n (Autor) Outra; miller, cj (Autor) Outra; sahlen, m (Autor) Outra; stanford, sa (Autor) Outra; stott, jp (Autor) Outra

Revista

Título: Monthly Notices of the Royal Astronomical Society

Vol. 422

Páginas: 1007-1013

ISSN: 0035-8711

Editora: Oxford University Press

Indexação

ISI Web of Knowledge - 4 Citações

Scopus - 4 Citações

Classificação Científica

FOS: Ciências exactas e naturais > Física

Outras Informações

ID Authenticus: P-002-AH0

DOI: 10.1111/j.1365-2966.2012.20673.x

Abstract (EN): 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 (Lambda CDM) 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.

Idioma: Inglês

Tipo (Avaliação Docente): Científica

Nº de páginas: 7