2015/12/14 by E. Pompei, C. Adami, D. Eckert +17 · 21 citations
Physics and Astronomy · #Active galactic nucleus #Astrophysics and Cosmic Phenomena #Background radiation #Cosmology #Dark matter #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Galaxy groups and clusters #Gamma-ray bursts and supernovae #Homogeneous #Universe #astro-ph.CO #astro-ph.GA
paper · pdf · doi:10.1051/0004-6361/201527142
published in Astronomy and Astrophysics 592, A6 (EDP Sciences) · A&A, accepted; special XXL issue
arxiv created 2015/12/14 · openalex publication_date 2015/12/15 · arxiv updated 2016/06/22 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
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.