Data

Australia Telescope Compact Array observations for project C3696 semester 2025OCTS

Commonwealth Scientific and Industrial Research Organisation
AJ, Nayana ; Laskar, Tanmoy ; Stroh, Michael ; Chornock, Ryan ; Margutti, Raffaella ; Terreran, Giacomo ; Sfaradi, Itai ; Wiston, Eli ; LeBaron, Natalie ; Brethauer, Daniel ; Hammerstein, Erica
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ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2FANDS&rft_id=https://data.csiro.au/collection/csiro:CASDA-ATOA-C3696-2025OCTS?tab=data DataDownload&rft.title=Australia Telescope Compact Array observations for project C3696 semester 2025OCTS&rft.identifier=https://data.csiro.au/collection/csiro:CASDA-ATOA-C3696-2025OCTS&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.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.&rft.creator=AJ, Nayana &rft.creator=Laskar, Tanmoy &rft.creator=Stroh, Michael &rft.creator=Chornock, Ryan &rft.creator=Margutti, Raffaella &rft.creator=Terreran, Giacomo &rft.creator=Sfaradi, Itai &rft.creator=Wiston, Eli &rft.creator=LeBaron, Natalie &rft.creator=Brethauer, Daniel &rft.creator=Hammerstein, Erica &rft.date=2025&rft.edition=v1&rft_rights=Creative Commons Attribution 4.0 International Licence https://creativecommons.org/licenses/by/4.0/&rft_rights=Data is accessible online and may be reused in accordance with licence conditions&rft_rights=All Rights (including copyright) CSIRO 2025.&rft_subject=supernovae&rft_subject=supernovae remnants&rft_subject=transients&rft_subject=Astronomical sciences not elsewhere classified&rft_subject=Astronomical sciences&rft_subject=PHYSICAL SCIENCES&rft.type=dataset&rft.language=English Access the data

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Creative Commons Attribution 4.0 International Licence
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Data is accessible online and may be reused in accordance with licence conditions

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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

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ACN 633 798 857