collaborators

9 papers

astro-ph.GA2026

The FAST HI 21-cm Absorption Blind Survey. III. OH Absorption Search in the 21-cm Absorber Sample and Continued HI Absorption Search

Wenkai Hu, Yougang Wang, Jeremy Darling +11

We present the first blind search for OH 18-cm absorption with the Five-hundred-meter Aperture Spherical Telescope (FAST), conducted alongside the HI 21-cm absorption search. Our p…

astro-ph.GA2026

Low-Frequency Recombination Lines from Galaxies and AGN over Cosmic Time

Kimberly L. Emig, Sergei Balashev, Francoise Combes +10

Radio recombination lines (RRLs) at low frequencies (<10 GHz) can provide a multi-phase view of interstellar gas in nearby galaxies, absorption-line-systems, and AGN. Hydrogen RRLs…

astro-ph.GA2026

Tracing Cold Gas in Absorption Across Cosmic Time with the SKA

Elizabeth K. Mahony, Neeraj Gupta, Sergei A. Balashev +12

Observing the 21-cm HI line in absorption provides a powerful means of tracing the cold neutral gas in normal and active galaxies across cosmic time. The frequency coverage and sen…

astro-ph.GA2026

The ASKAP-FLASH survey: A first look at the multiwavelength properties and redshift distribution of compact radio sources

W. Roster, E. M. Sadler, E. K. Mahony +15

We present the characterisation, including a photometric redshift (photo-) analysis, of the optical counterparts (CTPs) to over 45 000 bright ( 30 mJy) comp…

astro-ph.GA2025

RadioSED II: discovering the peaked spectrum radio sources in Stripe 82

E. F. Kerrison, E. M. Sadler, V. A. Moss +6

This paper is the second in a series presenting \textsc{RadioSED}, a Bayesian inference framework for constructing, modelling and classifying radio spectral energy distributions fr…

astro-ph.HE2025

A FLASH on Blazars: Capturing the Radio Realm of 4FGL Blazars with SKAO Pathfinders

Meriem Behiri, Elizabeth Mahony, Elaine Sadler +6

This work investigates the multi-wavelength properties of 165 4FGL blazars from the Fermi-LAT fourth source catalogue, looking for with counterparts in the Australian SKA Pathfinde…