Data

Australia Telescope Compact Array observations for project C3688 semester 2025OCTS

Commonwealth Scientific and Industrial Research Organisation
Sun, Xiaohui ; Yang, aiyuan ; Jing, Wenhui ; Gao, Xuyang
Viewed: [[ro.stat.viewed]] Cited: [[ro.stat.cited]] Accessed: [[ro.stat.accessed]]
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-C3688-2025OCTS?tab=data DataDownload&rft.title=Australia Telescope Compact Array observations for project C3688 semester 2025OCTS&rft.identifier=https://data.csiro.au/collection/csiro:CASDA-ATOA-C3688-2025OCTS&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=Supernova remnants (SNRs) drive interstellar turbulence and play an important role in the dynamic evolution of the Galaxy. Currently, there are about 300 known SNRs, and the number is far from complete. New surveys by JVLA, MeerKAT and ASKAP have found more than 400 SNR candidates, and the ongoing surveys by MeerKAT and ASKAP will find more. Confirming these candidates is now a pressing issue. We propose to observe a sample of small angular-size SNR candidates from the MeerKAT Galactic plane survey at C band with ATCA to observe their total intensity and polarization images. We will then derive the spectra of these SNR candidates with the C-band and MeerKAT images. The spectra, together with the polarization, will enable us to confirm these SNR candidates and obtain a confirmed SNR sample. This sample will help us assess the true number of SNRs in the Galaxy. The sample, containing mainly young SNRs, will also help to investigate the potential of SNRs being TeV-PeV accelerators.&rft.creator=Sun, Xiaohui &rft.creator=Yang, aiyuan &rft.creator=Jing, Wenhui &rft.creator=Gao, Xuyang &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=interstellar medium in and around the Milky Way&rft_subject=Astronomical sciences not elsewhere classified&rft_subject=Astronomical sciences&rft_subject=PHYSICAL SCIENCES&rft.type=dataset&rft.language=English Access the data

Licence & Rights:

Open Licence view details
CC-BY

Creative Commons Attribution 4.0 International Licence
https://creativecommons.org/licenses/by/4.0/

Data is accessible online and may be reused in accordance with licence conditions

All Rights (including copyright) CSIRO 2025.

Access:

Open view details

Accessible for free

Contact Information



Full description

Supernova remnants (SNRs) drive interstellar turbulence and play an important role in the dynamic evolution of the Galaxy. Currently, there are about 300 known SNRs, and the number is far from complete. New surveys by JVLA, MeerKAT and ASKAP have found more than 400 SNR candidates, and the ongoing surveys by MeerKAT and ASKAP will find more. Confirming these candidates is now a pressing issue. We propose to observe a sample of small angular-size SNR candidates from the MeerKAT Galactic plane survey at C band with ATCA to observe their total intensity and polarization images. We will then derive the spectra of these SNR candidates with the C-band and MeerKAT images. The spectra, together with the polarization, will enable us to confirm these SNR candidates and obtain a confirmed SNR sample. This sample will help us assess the true number of SNRs in the Galaxy. The sample, containing mainly young SNRs, will also help to investigate the potential of SNRs being TeV-PeV accelerators.

Available: 2025-11-28

Data time period: 2025-10-01 to 2026-04-01

Subjects

User Contributed Tags    

Login to tag this record with meaningful keywords to make it easier to discover

ACN 633 798 857