{ "id": "2307.09999", "version": "v1", "published": "2023-07-19T14:15:08.000Z", "updated": "2023-07-19T14:15:08.000Z", "title": "Searching for new globular clusters in M 31 with Gaia EDR3", "authors": [ "Yilun Wang", "Haibo Yuan", "Bingqiu Chen", "Xinlei Chen", "Hao Wu", "Zexi Niu", "Jifeng Li" ], "categories": [ "astro-ph.GA" ], "abstract": "We found 50 new globular cluster (GC) candidates around M\\,31 with Gaia Early Data Release 3 (EDR3), with the help from Pan-STARRS1 DR1 magnitudes and Pan-Andromeda Archaeological Survey (PAndAS) images. Based on the latest Revised Bologna Catalog and \\textit{simbad}, we trained 2 Random Forest (RF) classifiers, the first one to distinguish extended sources from point sources and the second one to further select GCs from extended sources. From 1.85 million sources of $16^m{<}g{<}19.5^m$ and within a large area of $\\sim$392\\,deg$^2$ around M\\,31, we selected 20,658 extended sources and 1,934 initial GC candidates. After visual inspection of the PAndAS images to eliminate the contamination of non-cluster sources, particularly galaxies, we finally got 50 candidates. These candidates are divided into 3 types (\\textbf{a}, \\textbf{b}, \\textbf{c}) according to their projected distance $D$ to the center of M\\,31 and their probability to be a true GC, $P_{GC}$, which is calculated by our second RF classifier. Among these candidates, 14 are found to be associated (in projection) with the large-scale structures within the halo of M\\,31. We also provided several simple parameter criteria for selecting extended sources effectively from the Gaia EDR3, which can reach a completeness of 92.1\\% with a contamination fraction lower than 10\\%.", "revisions": [ { "version": "v1", "updated": "2023-07-19T14:15:08.000Z" } ], "analyses": { "keywords": [ "gaia edr3", "globular cluster", "extended sources", "simple parameter criteria", "second rf classifier" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable" } } }