{ "id": "1802.06777", "version": "v1", "published": "2018-02-19T07:02:07.000Z", "updated": "2018-02-19T07:02:07.000Z", "title": "The selection function of the LAMOST Spectroscopic Survey of the Galactic Anticentre", "authors": [ "B. -Q. Chen", "X. -W. Liu", "H. -B. Yuan", "M. -S. Xiang", "Y. Huang", "C. Wang", "H. -W. Zhang", "Z. -J. Tian" ], "comment": "13 pages, 12 figures, accepted for publication in MNRAS", "categories": [ "astro-ph.GA", "astro-ph.SR" ], "abstract": "We present a detailed analysis of the selection function of the LAMOST Spectroscopic Survey of the Galactic Anti-centre (LSS-GAC). LSS-GAC was designed to obtain low resolution optical spectra for a sample of more than 3 million stars in the Galactic anti-centre. The second release of value-added catalogues of the LSS-GAC (LSS-GAC DR2) contains stellar parameters, including radial velocity, atmospheric parameters, elemental abundances and absolute magnitudes deduced from 1.8 million spectra of 1.4 million unique stars targeted by the LSS-GAC between 2011 and 2014. For many studies using this database, such as those investigating the chemodynamical structure of the Milky Way, a detailed understanding of the selection function of the survey is indispensable. In this paper, we describe how the selection function of the LSS-GAC can be evaluated to sufficient detail and provide selection function corrections for all spectroscopic measurements with reliable parameters released in LSS-GAC DR2. The results, to be released as new entries in the LSS-GAC value-added catalogues, can be used to correct the selection effects of the catalogue for scientific studies of various purposes.", "revisions": [ { "version": "v1", "updated": "2018-02-19T07:02:07.000Z" } ], "analyses": { "keywords": [ "lamost spectroscopic survey", "galactic anticentre", "galactic anti-centre", "lss-gac dr2", "selection function corrections" ], "note": { "typesetting": "TeX", "pages": 13, "language": "en", "license": "arXiv", "status": "editable" } } }