{ "id": "1604.01314", "version": "v1", "published": "2016-04-05T16:08:42.000Z", "updated": "2016-04-05T16:08:42.000Z", "title": "On the faint-end of the high-$z$ galaxy luminosity function", "authors": [ "Bin Yue", "Andrea Ferrara", "Yidong Xu" ], "comment": "11 pages, 13 figures, submitted to MNRAS", "categories": [ "astro-ph.GA", "astro-ph.CO" ], "abstract": "Recent measurement of the Luminosity Function (LF) of galaxies in the Epoch of Reionization (EoR, redshift $z>6$) indicates a very steep increase of the number density of low-mass galaxies populating the LF faint-end. As star formation in such systems can be easily quenched by radiative feedback effects, a turn-off is expected at some faint magnitude. Using a physically-motivated analytical model, we quantify reionization feedback effects on the LF. If reionization feedback is neglected, the power-law Schechter parameterization characterizing the faint-end of the LF remains valid up to $M_{\\rm UV}\\sim -9$. If (strong) feedback is included, the LF drops above $M_{\\rm UV} \\sim -15$, slightly below the detection limit of current surveys at $z\\sim5$. However, the LF may rise again at higher $M_{\\rm UV}$ as a result of the interplay between reionization topology and photo-evaporation physics. Moreover, we find that the stellar age -- magnitude relation might be used as a probe of feedback strength as well: in models with stronger reionization feedback, stars in galaxies with $-13 \\lsim M_{\\rm UV} \\lsim -8$ are typically older. Other suggested constraints on feedback can come from galaxy number counts data, particularly those exploiting gravitational lensing magnification.", "revisions": [ { "version": "v1", "updated": "2016-04-05T16:08:42.000Z" } ], "analyses": { "keywords": [ "galaxy luminosity function", "galaxy number counts data", "stronger reionization feedback", "quantify reionization feedback effects", "power-law schechter parameterization" ], "note": { "typesetting": "TeX", "pages": 11, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2016arXiv160401314Y", "inspire": 1442335 } } }