Home > Research > Publications & Outputs > The XMM Cluster Survey

Associated organisational unit

View graph of relations

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

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Published

Standard

The XMM Cluster Survey: Predicted overlap with the Planck Cluster Catalogue. / Viana, Pedro T. P.; Da Silva, António; Ramos, Elsa P. R. G. et al.
In: Monthly Notices of the Royal Astronomical Society, Vol. 422, No. 2, 11.05.2012, p. 1007-1013.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Viana, PTP, Da Silva, A, Ramos, EPRG, Liddle, AR, Lloyd-Davies, EJ, Romer, AK, Kay, ST, Collins, CA, Hilton, M, Hosmer, M, Hoyle, B, Mayers, JA, Mehrtens, N, Miller, CJ, Sahlén, M, Stanford, SA & Stott, JP 2012, 'The XMM Cluster Survey: Predicted overlap with the Planck Cluster Catalogue', Monthly Notices of the Royal Astronomical Society, vol. 422, no. 2, pp. 1007-1013. https://doi.org/10.1111/j.1365-2966.2012.20673.x

APA

Viana, P. T. P., Da Silva, A., Ramos, E. P. R. G., Liddle, A. R., Lloyd-Davies, E. J., Romer, A. K., Kay, S. T., Collins, C. A., Hilton, M., Hosmer, M., Hoyle, B., Mayers, J. A., Mehrtens, N., Miller, C. J., Sahlén, M., Stanford, S. A., & Stott, J. P. (2012). The XMM Cluster Survey: Predicted overlap with the Planck Cluster Catalogue. Monthly Notices of the Royal Astronomical Society, 422(2), 1007-1013. https://doi.org/10.1111/j.1365-2966.2012.20673.x

Vancouver

Viana PTP, Da Silva A, Ramos EPRG, Liddle AR, Lloyd-Davies EJ, Romer AK et al. The XMM Cluster Survey: Predicted overlap with the Planck Cluster Catalogue. Monthly Notices of the Royal Astronomical Society. 2012 May 11;422(2):1007-1013. Epub 2012 Apr 25. doi: 10.1111/j.1365-2966.2012.20673.x

Author

Viana, Pedro T. P. ; Da Silva, António ; Ramos, Elsa P. R. G. et al. / The XMM Cluster Survey : Predicted overlap with the Planck Cluster Catalogue. In: Monthly Notices of the Royal Astronomical Society. 2012 ; Vol. 422, No. 2. pp. 1007-1013.

Bibtex

@article{bd625569a34c4e83865cd1de90fcdf3f,
title = "The XMM Cluster Survey: Predicted overlap with the Planck Cluster Catalogue",
abstract = "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.",
keywords = "Galaxies: clusters: general",
author = "Viana, {Pedro T. P.} and {Da Silva}, Ant{\'o}nio and Ramos, {Elsa P. R. G.} and Liddle, {Andrew R.} and Lloyd-Davies, {E. J.} and Romer, {A. Kathy} and Kay, {Scott T.} and Collins, {Chris A.} and Matt Hilton and Mark Hosmer and Ben Hoyle and Mayers, {Julian A.} and Nicola Mehrtens and Miller, {Christopher J.} and Martin Sahl{\'e}n and Stanford, {S. Adam} and Stott, {John P.}",
year = "2012",
month = may,
day = "11",
doi = "10.1111/j.1365-2966.2012.20673.x",
language = "English",
volume = "422",
pages = "1007--1013",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "OXFORD UNIV PRESS",
number = "2",

}

RIS

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 -