{ "id": "2204.11883", "version": "v1", "published": "2022-04-25T18:00:08.000Z", "updated": "2022-04-25T18:00:08.000Z", "title": "The Nature of Low Surface Brightness Galaxies in the Hyper Suprime-Cam Survey", "authors": [ "Jenny E Greene", "Johnny P. Greco", "Andy D. Goulding", "Song Huang", "Erin Kado-Fong", "Shany Danieli", "Jiaxuan Li", "Ji Hoon Kim", "Yutaka Komiyama", "Alexie Leauthaud", "Lauren A. MacArthur", "Cristobal Sifon" ], "comment": "15 pages, 6 figures, resubmitted to ApJ after review", "categories": [ "astro-ph.GA" ], "abstract": "We present the statistical redshift distribution of a large sample of low surface brightness (LSB) galaxies identified in the first 200 deg$^2$ of the Hyper Suprime-Cam Strategic Survey Program. Through cross-correlation with the NASA-SDSS Atlas, we find that the majority of objects lie within z<0.15 or ~ 500 Mpc, yielding a mass range of $M_*$ ~ $10^7-10^9$ M_sun and size range of $r_{\\rm{eff,g}}$ ~ 1-8 kpc. We find a peak in the distance distribution within 100 Mpc, corresponding mostly to ~ $10^7$ M_sun galaxies that fall on the known mass-size relation. There is also a tail in the redshift distribution out to z~0.15, comprising more massive ($M_*=10^8-10^9$ M_sun) galaxies at the larger end of our size range. We see tentative evidence that at the higher-mass end ($M_* > 10^8$ M_sun) the LSB galaxies do not form a smooth extension of the mass-size relation of higher surface brightness galaxies, perhaps suggesting that the LSB galaxy population is distinct in its formation path.", "revisions": [ { "version": "v1", "updated": "2022-04-25T18:00:08.000Z" } ], "analyses": { "keywords": [ "low surface brightness galaxies", "hyper suprime-cam survey", "hyper suprime-cam strategic survey program", "higher surface brightness galaxies", "redshift distribution" ], "note": { "typesetting": "TeX", "pages": 15, "language": "en", "license": "arXiv", "status": "editable" } } }