{ "id": "1603.03260", "version": "v1", "published": "2016-03-10T13:37:46.000Z", "updated": "2016-03-10T13:37:46.000Z", "title": "Compatibility of the Large Quasar Groups with the Concordance Cosmological Model", "authors": [ "Gabriel E. Marinello", "Roger G. Clowes", "Luis E. Campusano", "Gerald M. Williger", "Ilona K. Söchting", "Matthew J. Graham" ], "comment": "16 pages, 12 figures, Submitted in MNRAS", "categories": [ "astro-ph.CO" ], "abstract": "We study the compatibility of large quasar groups with the concordance cosmological model. Large Quasar Groups are very large spatial associations of quasars in the cosmic web, with sizes of 50-250h^-1 Mpc. In particular, the largest large quasar group known, named Huge-LQG, has a longest axis of ~860h^-1 Mpc, larger than the scale of homogeneity (~260 Mpc), which has been pointed as a possible violation of the cosmological principle. Using mock catalogues constructed from the Horizon Run 2 cosmological simulation, we found that large quasar groups size, quasar member number and mean overdensity distributions in the mocks agree with observations. The Huge-LQG is found to be a rare group with a probability of 0.3 per cent of finding a group as large or larger than the observed, but an extreme value analysis shows that it is an expected maximum in the sample volume with a probability of 19 per cent of observing a largest quasar group as large or larger than Huge-LQG. The Huge-LQG is expected to be the largest structure in a volume at least 5.3 +- 1 times larger than the one currently studied.", "revisions": [ { "version": "v1", "updated": "2016-03-10T13:37:46.000Z" } ], "analyses": { "keywords": [ "concordance cosmological model", "compatibility", "largest large quasar group", "quasar member number", "extreme value analysis" ], "note": { "typesetting": "TeX", "pages": 16, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2016arXiv160303260M", "inspire": 1427000 } } }