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19982013
most citedA Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34

609 citations · 1.5k across the 12 of their papers we have counts for

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14 papers · 1 filter

astro-ph2006

A 15um selected sample of high-z starbursts and AGNs

A. Hernan-Caballero, I. Perez-Fournon, M. Rowan-Robinson +19

We report results from a Spitzer GO-1 program of IRS spectroscopy of a large sample of Luminous Infrared Galaxies and quasars selected from the European Large Area ISO Survey (ELAI…

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

Rotation of the cluster of galaxies A2107

M. Kalinkov, T. Valchanov, I. Valtchanov +2

We present indications of rotation in the galaxy cluster A2107 by a method that searches for the maximum gradient in the velocity field in a flat disk-like model of a cluster. Gala…