{ "id": "2204.00831", "version": "v1", "published": "2022-04-02T10:44:47.000Z", "updated": "2022-04-02T10:44:47.000Z", "title": "Estimation of the Star Formation Rate of Galaxies with Radio Continuum Obtained with Murchison Widefield Array", "authors": [ "Tsutomu T. Takeuchi", "Shuntaro A. Yoshida", "Luca Cortese", "O. Ivy Wong", "Barbara Catinella", "Suchetha Cooray" ], "comment": "13 pages, 6 figures, 2 tables, submitted", "categories": [ "astro-ph.GA" ], "abstract": "We investigate the correlation between the integrated low-frequency and infrared (IR) emissions of star-forming galaxies extracted from the {\\sl Herschel} Reference Survey. By taking advantage of the GaLactic Extragalactic All-sky MWA (GLEAM) survey operated by the Murchison Widefield Array (MWA) we examine how this correlation varies at a function of frequency across the 20 GLEAM narrow bands at $72\\mbox{--}231\\; [\\mbox{MHz}]$. These examinations are important for ensuring the reliability of the radio luminosity as a SFR indicator. In this study, we focus on 18 star-forming galaxies whose radio emission is detected by the GLEAM survey. These galaxies show that a single power-law is sufficient to characterise the far-infrared-to-radio correlation across the GLEAM frequency bands and up to $1.5\\; [\\mbox{GHz}]$. Thus, the radio continuum in this wavelength range can serve as a good dust extinction-free SFR estimator. This is particularly important for future investigation of the cosmic SFR independently from other estimators, since the radio continuum can be detected from $z=0$ to high redshifts ($z \\sim 5\\mbox{--}10$) in a coherent manner.", "revisions": [ { "version": "v1", "updated": "2022-04-02T10:44:47.000Z" } ], "analyses": { "keywords": [ "murchison widefield array", "radio continuum", "star formation rate", "estimation", "dust extinction-free sfr estimator" ], "note": { "typesetting": "TeX", "pages": 13, "language": "en", "license": "arXiv", "status": "editable" } } }