Full description
Radio and X-ray observations of supernovae (SNe) years to decades post-explosion are crucial to drive progress in several fundamental areas of explosive transient research. Key questions include the nature of mass-loss preceding explosions, progenitor star attributes leading to central engines, and the properties of young neutron stars and black holes. However, there are very limited subsets of SNe with late-time radio observations. We developed a sample of 14 X-ray sources from the SRG/eROSITA all-sky survey data at the location of known core-collapse SNe, offering new avenues for exploration. We propose a pilot ATCA survey of six X-ray sources from this sample to investigate their late-time radio evolution as part of a broader multi-wavelength follow-up campaign. We request 66 hours of ATCA time for this project.Available: 2025-11-28
Data time period: 2025-10-01 to 2026-04-01
Subjects
Astronomical Sciences |
Astronomical Sciences Not Elsewhere Classified |
Physical Sciences |
supernovae |
supernovae remnants |
transients |
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