{ "id": "2309.11559", "version": "v1", "published": "2023-09-20T18:00:47.000Z", "updated": "2023-09-20T18:00:47.000Z", "title": "A Close Look at Ly$α$ Emitters with JWST/NIRCam at $z\\approx3.1$", "authors": [ "Yixiao Liu", "Y. Sophia Dai", "Stijn Wuyts", "Jia-Sheng Huang", "Linhua Jiang" ], "comment": "16 pages, 6 figures, submitted to ApJ", "categories": [ "astro-ph.GA" ], "abstract": "We study 10 spectroscopically confirmed Ly$\\alpha$ emitters (LAEs) at $z\\approx3.1$ in the UDS field, covered by JWST/NIRCam in the PRIMER program. All LAEs are detected in all NIRCam bands from F090W to F444W, corresponding to restframe 2200\\AA--1.2$\\mathrm{\\mu m}$. Based on morphological analysis of the F200W images, three out of the 10 targets are resolved into pair-like systems with separations of $<0.9''$, and another three show asymmetric structures. We then construct the spectral energy distributions (SEDs) of these LAEs. All sources, including the pairs, show similar SED shapes, with a prominent flux excess in the F200W band, corresponding to extremely strong [O III]+H$\\beta$ emission lines (${\\rm EW_{rest}}=740$--$6500\\,$\\AA). The median effective radii, stellar mass, and UV slope of our sample are 0.36$\\,$kpc, $3.8\\times10^7\\,M_\\odot$, and --2.48, respectively. The average burst age, estimated by stellar mass over star formation rate, is $<40\\,$Myr. These measurements reveal an intriguing starbursting dwarf galaxy population lying off the extrapolations of the $z \\sim 3$ scaling relations to the low-mass end: $\\sim 0.7$ dex above the star-forming main sequence, $\\sim 0.35$ dex below the mass--size relation, and bluer in the UV slope than typical high-z galaxies at similar UV luminosities. We speculate that these numbers may require a larger main sequence scatter or tail in the dwarf galaxy regime towards the starburst outliers.", "revisions": [ { "version": "v1", "updated": "2023-09-20T18:00:47.000Z" } ], "analyses": { "keywords": [ "close look", "starbursting dwarf galaxy population", "dwarf galaxy population lying", "jwst/nircam", "stellar mass" ], "note": { "typesetting": "TeX", "pages": 16, "language": "en", "license": "arXiv", "status": "editable" } } }