The host galaxy and persistent radio counterpart of FRB 20201124A. Issue 1 (25th April 2022)

• Record Type: Journal Article
• Authors: Ravi, Vikram; Law, Casey J; Li, Dongzi; Aggarwal, Kshitij; Bhardwaj, Mohit; Burke-Spolaor, Sarah; Connor, Liam; Lazio, T Joseph W; Simard, Dana; Somalwar, Jean; Tendulkar, Shriharsh P
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 513:Issue 1(2022)
• Page Start: 982
• Page End: 990
• Publication Date: 2022-04-25
• Subjects: galaxies: star formation -- radio continuum: galaxies -- radio continuum: transients -- fast radio bursts; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stac465
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: The physical properties of fast radio burst (FRB) host galaxies provide important clues towards the nature of FRB sources. The 16 FRB hosts identified thus far span three orders of magnitude in mass and specific star formation rate, implicating a ubiquitously occurring progenitor object. FRBs localized with ∼arcsecond accuracy also enable effective searches for associated multiwavelength and multi-time-scale counterparts, such as the persistent radio source associated with FRB 20121102A. Here we present a localization of the repeating source FRB 20201124A, and its association with a host galaxy (SDSS J050803.48+260338.0, z = 0.098) and persistent radio source. The galaxy is massive (${\sim}3\times 10^{10}\, \text{M}_{\odot }$ ), star-forming (few solar masses per year), and dusty. Very Large Array and Very Long Baseline Array observations of the persistent radio source measure a luminosity of 1.2 × 10 29 erg s −1 Hz −1, and show that is extended on scales ≳50 mas. We associate this radio emission with the ongoing star formation activity in SDSS J050803.48+260338.0. Deeper, high-resolution optical observations are required to better utilize the milliarcsecond-scale localization of FRB 20201124A and determine the origin of the large dispersion measure (150–220 pc cm −3 ) contributed by the host. SDSS J050803.48+260338.0 is an order of magnitude more massive than any galaxy or stellar system previously associated with a repeating FRB source, but is comparable to the hosts of so far non-repeating FRBs, further building the link between the two apparent populations.