The XXL Survey
Maggie LieuSchool of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham, B15 2TT, UKG. P. SmithSchool of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham, B15 2TT, UKPaul GilesH. H. Wills Physics Laboratory, University of Bristol, Tyndall Avenue, Bristol, BS8 1TL, UKF. ZiparoSchool of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham, B15 2TT, UKB. J. MaughanH. H. Wills Physics Laboratory, University of Bristol, Tyndall Avenue, Bristol, BS8 1TL, UKJ. DémoclèsSchool of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham, B15 2TT, UKF. PacaudArgelander Institut für Astronomie, Universität Bonn, 53121 Bonn, GermanyM. PierreService d’Astrophysique AIM, CEA Saclay, 91191 Gif-sur-Yvette, FranceC. AdamiUniversité Aix Marseille, CNRS, LAM (Laboratoire d’Astrophysique de Marseille) UMR 7326, 13388 Marseille, FranceYannick M BahéInstitute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UKN. ClercMax Planck Institut für Extraterrestrische Physik, Postfach 1312, 85741 Garching bei München, GermanyL. ChiappettiINAF–IASF-Milano, via E. Bassini 15, 20133 Milano, ItalyD. EckertDepartment of Astronomy, University of Geneva, ch. d’Ecogia 16, 1290 Versoix, SwitzerlandS. EttoriINAF–Osservatorio Astronomico di Bologna, via Ranzani 1, 40127 Bologna, ItalyS. LavoieDepartment of Physics and Astronomy, University of Victoria, 3800 Finnerty Road, Victoria, BC, V8P 1A1, CanadaJ. P. Le FèvreSEDI CEA Saclay, FranceIan G. McCarthyAstrophysics Research Institute, Liverpool John Moores University, IC2, 146 Brownlow Hill, Liverpool L3 5RF, UKM. KilbingerService d’Astrophysique AIM, CEA Saclay, 91191 Gif-sur-Yvette, FranceT. J. PonmanSchool of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham, B15 2TT, UKT. SadibekovaService d’Astrophysique AIM, CEA Saclay, 91191 Gif-sur-Yvette, FranceJ. P. WillisInstitute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
2015en
ABI
Аннотация
Context. The XXL Survey is the largest survey carried out by XMM-Newton. Covering an area of 50 deg2, the survey contains ~450 galaxy clusters out to a redshift ~2 and to an X-ray flux limit of ~ 5 × 10-15 erg s-1 cm-2. This paper is part of the first release of XXL results focussed on the bright cluster sample.
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