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most citedThe XMM Large Scale Structure survey: The X-ray pipeline and survey selection function

116 citations · 247 across the 4 of their papers we have counts for

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astro-ph20082 cited

XMMU J134736.6+173403: an eclipsing LMXB in quiescence or a peculiar AGN?

S. Carpano, B. Altieri, A. R. King +2

Aims. We report the discovery of a peculiar object observed serendipitously with XMM-Newton. We present its timing and spectral properties and investigate its optical counterpart.…

astro-ph200665 cited

XMM-LSS discovery of a z=1.22 galaxy cluster

M. N. Bremer, I. Valtchanov, J. P. Willis +11

We present details of the discovery of XLSSJ022303.0-043622, a z=1.2 cluster of galaxies. This cluster was identified from its X-ray properties and selected as a z>1 candidate from…

astro-ph2006116 cited

The XMM Large Scale Structure survey: The X-ray pipeline and survey selection function

F. Pacaud, M. Pierre, A. Refregier +11

We present the X-ray pipeline developed for the purpose of the cluster search in the XMM-LSS survey. It is based on a two-stage procedure via a dedicated handling of the Poisson na…

astro-ph200664 cited

The XMM-LSS Survey: A well controlled X-ray cluster sample over the D1 CFHTLS area

M. Pierre, F. Pacaud, P. -A. Duc +24

We present the XMM-LSS cluster catalogue corresponding to the CFHTLS D1 area. The list contains 13 spectroscopically confirmed, X-ray selected galaxy clusters over 0.8 deg2 to a re…

astro-ph2005

The XMM Large-Scale Structure Survey: An initial sample of galaxy groups and clusters to a redshift z<0.6

J. P. Willis, F. Pacaud, I. Valtchanov +14

We present X-ray and optical spectroscopic observations of twelve galaxy groups and clusters identified within the XMM Large-Scale Structure (LSS) survey. Groups and clusters are s…

astro-ph2005

Batch discovery of nine z~1 clusters using x-ray and K or R,z' images

S. Andreon, I. Valtchanov, L. R. Jones +5

We present results of an initial search for clusters of galaxies at z~1 and above, using data from 2.9 square degrees of XMM-Newton images. By selecting weak potentially extended X…