Tracing cosmic star formation history through radio continuum spectral energy distribution and non-thermal emission

arXiv:2607.12073 · astro-ph.GA · Submitted 2026-07-13 · Read on arXiv

Fangxia An, Fatemeh S. Tabatabaei, Nick Seymour, Maryam Khademi, Zunli Yuan, Wenjie Wang, Joe A. Grundy, Mark T. Sargent, Tao Wang, Yuheng Zhang, Yinghe Zhao, Hiddo S. B. Algera, Elias Brinks, Mattia Vaccari

astro-ph.GA

Submitted: 2026-07-13

Comments: Published in Advancing Astrophysics with the SKA II (AASKAII),2026 (arXiv:2606.20366). Report-no:AASKAII/FangxiaAn01

License: http://creativecommons.org/licenses/by-nc-sa/4.0/

The gist: As a tracer of massive star formation unaffected by dust, the radio continuum emission provides a unique window into the formation of the first stars and galaxies in the Universe.

Terminology

Abstract

As a tracer of massive star formation unaffected by dust, the radio continuum emission provides a unique window into the formation of the first stars and galaxies in the Universe. Recent observations show that the integrated rest-frame mid-radio (1-10 GHz) luminosity of galaxies serves as one of the most robust tracers of the star formation rate (SFR). These studies further demonstrate that the synchrotron spectral index and the shape of the radio spectral energy distribution (SED) evolves with redshift as a consequence of the cosmic evolution of star formation activity. These findings underscore the importance of deep multi-band radio continuum observations in calibrating the SFR of early galaxies and understanding the astrophysical processes governing their assembly and evolution over cosmic time. This chapter presents recent progress in radio SFR calibrations for star-forming galaxies (SFGs) and reviews radio-continuum studies of the cosmic star formation history (SFH). We highlight the transformative potential of SKA AA4, whose broad frequency coverage and high sensitivity will enable well-constrained radio SEDs for SFGs across a wide redshift range.

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