The XXL Survey
E. PompeiC. AdamiAix Marseille Université, CNRS, LAM (Laboratoire d’Astrophysique de Marseille), UMR 7326, 13388 Marseille, FranceD. EckertDepartment of Astronomy, University of Geneva, ch. d’Ecogia 16, 1290 Versoix, SwitzerlandF. GastaldelloINAF–IASF-Milano, via Bassini 15, 20133 Milano, Italy Department of Physics and Astronomy, University of California at Irvine, USAS. LavoieDepartment of Physics and Astronomy, University of Victoria, 3800 Finnerty Road, Victoria, BC, CanadaB. PoggiantiOsservatorio astronomico di Padova, INAF, 35141 Padova, ItalyB. AltieriEuropean Space Astronomy Centre, European Space Agency, PO Box 78, 28691 Villanueva de la Cañada, Madrid, SpainS. AlisDepartment of Astronomy and Space Sciences, Faculty of Science, Istanbul University, 34119 Istanbul, TurkeyN. BaranDepartment of Physics, University of Zagreb, Bijenička cesta 32, 45 10000 Zagreb, CroatiaC. BenoistLaboratoire Lagrange, UMR 7293, Université de Nice Sophia Antipolis, CNRS, Observatoire de la Cote d’Azur, 06304 Nice, FranceY. L. JafféDepartment of Astronomy, Universidad de Concepción, Casilla 160-C, Concepción, ChileE. KoulouridisIAASARS, National Observatory of Athens, 15236 Penteli, GreeceS. MaurogordatoLaboratoire Lagrange, UMR 7293, Université de Nice Sophia Antipolis, CNRS, Observatoire de la Cote d’Azur, 06304 Nice, FranceF. PacaudArgelander Institut für Astronomie, Universitat Bonn, 53121 Bonn, GermanyM. PierreService d’Astrophysique AIM, CEA/DSM/IRFU/SAp, CEA Saclay, 91191 Gif-sur-Yvette, FranceT. SadibekovaService d’Astrophysique AIM, CEA/DSM/IRFU/SAp, CEA Saclay, 91191 Gif-sur-Yvette, FranceV. SmolčićDepartment of Physics, University of Zagreb, Bijenička cesta 32, 45 10000 Zagreb, CroatiaI. ValtchanovEuropean Space Astronomy Centre, European Space Agency, PO Box 78, 28691 Villanueva de la Cañada, Madrid, Spain
2015en
ABI
Аннотация
Context. The XXL Survey is the largest homogeneous and contiguous survey carried out with XMM-Newton. Covering an area of 50 deg2 distributed over two fields, it primarily investigates the large-scale structures of the Universe using the distribution of galaxy clusters and active galactic nuclei as tracers of the matter distribution.
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