{ "id": "2101.07827", "version": "v1", "published": "2021-01-19T19:18:20.000Z", "updated": "2021-01-19T19:18:20.000Z", "title": "Source Counts Spanning Eight Decades of Flux Density at 1.4 GHz", "authors": [ "A. M. Matthews", "J. J. Condon", "W. D. Cotton", "T. Mauch" ], "comment": "19 pages, 13 figures, accepted for publication in ApJ", "categories": [ "astro-ph.GA" ], "abstract": "Brightness-weighted differential source counts $S^2 n(S)$ spanning the eight decades of flux density between $0.25\\,\\mu\\mathrm{Jy}$ and 25 Jy at 1.4 GHz were measured from (1) the confusion brightness distribution in the MeerKAT DEEP2 image below $10\\,\\mu\\mathrm{Jy}$, (2) counts of DEEP2 sources between $10\\,\\mu\\mathrm{Jy}$ and $2.5\\,\\mathrm{mJy}$, and (3) counts of NVSS sources stronger than $2.5\\,\\mathrm{mJy}$. We present our DEEP2 catalog of $1.7 \\times 10^4$ discrete sources complete above $S = 10\\,\\mu\\mathrm{Jy}$ over $\\Omega = 1.04\\,\\mathrm{deg}^2$. The brightness-weighted counts converge as $S^2 n(S) \\propto S^{1/2}$ below $S = 10\\,\\mu\\mathrm{Jy}$, so $>99\\%$ of the $\\Delta T_\\mathrm{b} \\sim 0.06\\,\\mathrm{K}$ sky brightness produced by active galactic nuclei and $\\approx96\\%$ of the $\\Delta T_\\mathrm{b} \\sim 0.04\\,\\mathrm{K}$ added by star-forming galaxies has been resolved into sources with $S \\geq 0.25\\,\\mu\\mathrm{Jy}$. The $\\Delta T_\\mathrm{b} \\approx 0.4\\,\\mathrm{K}$ excess brightness measured by ARCADE 2 cannot be produced by faint sources smaller than $\\approx 50\\,\\mathrm{kpc}$ if they cluster like galaxies.", "revisions": [ { "version": "v1", "updated": "2021-01-19T19:18:20.000Z" } ], "analyses": { "keywords": [ "flux density", "source counts spanning", "faint sources smaller", "confusion brightness distribution", "meerkat deep2 image" ], "note": { "typesetting": "TeX", "pages": 19, "language": "en", "license": "arXiv", "status": "editable" } } }