Radio transients and variables in the tenth Deeper, Wider, Faster observing run. Issue 3 (24th December 2022)

• Record Type: Journal Article
• Authors: Dobie, D; Pritchard, J; Wang, Y; Graham, L W; Freeburn, J; Qiu, H; White, T R; O'Brien, A; Lenc, E; Leung, J K; Lynch, C; Murphy, Tara; Stewart, A J; Wang, Z; Zic, A; Abbott, T M C; Cai, C; Cooke, J; Dobiecki, M; Goode, S; Jia, S; Li, C; Möller, A; Webb, S; Zhang, J; Zhang, S N
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 519:Issue 3(2023)
• Page Start: 4684
• Page End: 4698
• Publication Date: 2022-12-24
• Subjects: polarization -- stars: flare -- stars: low-mass -- radio continuum: transients -- radio continuum: stars; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stac3731
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: The Deeper, Wider, Faster (DWF) program coordinates observations with telescopes across the electromagnetic spectrum, searching for transients on time-scales of milliseconds to days. The tenth DWF observing run was carried out in near real-time during September 2021, and consisted of six consecutive days of observations of the NGC 6744 galaxy group and a field containing the repeating fast radio burst FRB 190711 with the Australian Square Kilometre Array Pathfinder, the Dark Energy Camera, the Hard X-ray Modulation Telescope, and the Parkes 64-m 'Murriyang' radio telescope. In this work, we present the results of an image-domain search for transient, variable, and circularly polarized sources carried out with ASKAP, using data from the observing run along with test observations prior to the run and follow-up observations carried out during and after the run. We identified eight variable radio sources, consisting of one pulsar, six stellar systems (five of which exhibit circularly polarized emission), and one previously uncatalogued source. Of particular interest is the detection of pulses from the ultra-cool dwarf SCR J1845–6357 with a period of 14.2 ± 0.3 h in good agreement with the known optical rotation period, making this the slowest rotating radio-loud ultra-cool dwarf discovered.