{ "id": "1809.08244", "version": "v1", "published": "2018-09-21T18:00:02.000Z", "updated": "2018-09-21T18:00:02.000Z", "title": "New ultra-cool and brown dwarf candidates in Gaia DR2", "authors": [ "C. Reylé" ], "comment": "accepted for publication in A&A, 9 pages", "categories": [ "astro-ph.SR" ], "abstract": "Context. The second Gaia data release (Gaia DR2) contains high precision positions, parallaxes and proper motions for 1.3 billion sources. The resulting Hertzsprung-Russel diagram reveals fine structures all over the mass range. Aims. This paper aims to investigate the content of Gaia DR2 at the low-mass end and to characterize ultra-cool and brown dwarfs. Methods. We first retrieve the sample of spectroscopically confirmed ultra-cool and brown dwarfs in Gaia DR2. We use their locus in the precise Hertzsprung-Russel diagram to select new candidates, and to investigate their properties. Results. The number of spectroscopically confirmed objects recovered in Gaia DR2 corresponds to 62 %, and 71 %, of the expected number of objects with and estimated Gaia magnitude Gest $\\leq$ 21.5, and 20.3, respectively, significantly filling the gap with Gaia DR1. Furthermore Gaia DR2 contains ~13 000 $\\geq$M7 and 679 new L candidates. A tentative classification suggests that a few hundreds are young or subdwarf candidates. Their distance distribution shows that the solar neighborhood census is still incomplete. Conclusions. Gaia DR2 offers a great wealth of information on the low-mass objects. It provide a homogeneous and precise catalog of candidates worthwhile to be further characterized with spectroscopic observations.", "revisions": [ { "version": "v1", "updated": "2018-09-21T18:00:02.000Z" } ], "analyses": { "keywords": [ "brown dwarf candidates", "ultra-cool", "contains high precision positions", "gaia dr2 offers", "second gaia data" ], "note": { "typesetting": "TeX", "pages": 9, "language": "en", "license": "arXiv", "status": "editable" } } }