In this episode, we dive into how astronomers are combining the power of the Australian Square Kilometre Array Pathfinder (ASKAP) and the Vera C. Rubin Observatory to capture the dynamic, ever-changing sky in real time.
Historically, optical and gravitational-wave observatories issued rapid alerts, but radio astronomy lacked automated, large-scale, real-time alert infrastructure. Now, a long-term monitoring program (project AS331) targets Rubin’s Deep Drilling Fields (DDFs), taking 3-hour radio snapshots approximately every 10 days to achieve a sensitivity of \\(\sim 60\ \mu\text{Jy}\\). This complementary survey automatically processes and streams radio data to the global astronomical community in near-real-time without human intervention.
Episode Highlights & Key Discoveries:
Bridging Optical and Radio Astronomy: How contemporaneous, non-coordinated radio surveys solve the bottleneck of follow-up observations for millions of optical alerts.
Tidal Disruption Events (TDEs): Updated high-cadence light curves for AT2018hyz, revealing late-time radio flaring and scintillation effects that constrain the outflow size.
Supernova Interaction: Modelling circumstellar material interactions around the Type IIb supernova SN2024abfo.
New Cosmic Discoveries: The detection of ASKAP J095711.5+051205 (a candidate optical-less TDE in a poststarburst galaxy) and ASKAP J005026.4-422958 (an ongoing Extreme Scattering Event caused by plasma lensing).
### Article Reference
Title: ASKAP Monitoring of the Rubin Deep Drilling Fields
Authors: Dougal Dobie, James Freeburn, Iris de Ruiter, Katie Auchettl, James Coulson, Brent Miszalski, Anais Möller, and Nikhil Sarin
Identifier: arXiv:2610.13011v1
Acknowledements: Podcast prepared with Google/Gemini Notebook. Illustration credits: CSIRO
Podden och tillhörande omslagsbild på den här sidan tillhör
Astro-COLIBRI. Innehållet i podden är skapat av Astro-COLIBRI och inte av,
eller tillsammans med, Poddtoppen.