Supernova Remnant Candidates Discovered by the SARAO MeerKAT Galactic Plane Survey

L. D. Anderson, F. Camilo, Timothy Faerber, M. Bietenholz, C. Bordiu, F. Bufano, J. O. Chibueze, W. D. Cotton, A. Ingallinera, S. Loru, A. Rigby, S. Riggi, M. A. Thompson, G. Umana, G. M. Williams (2024): Supernova Remnant Candidates Discovered by the SARAO MeerKAT Galactic Plane Survey, South African Radio Astronomy Observatory, https://doi.org/10.48479/0n8c-5q84

Data release for Supernova Remnant Candidates Discovered by the SARAO MeerKAT Galactic Plane Survey, Anderson et al. (2024) (link to paper).

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Images PDF images for each SNR or SNR candidate mentioned in the text. For each image, MIR data are in the left panels (Spitzer or WISE) and SMGPS 1.3 GHz data are on the right. White circles show HII regions from the WISE Catalog, blue-green circles show previously-known SNRs (filenames begin with "Known_Green" or "Known_SNRCat"), green circles show previously-known SNR candidates ("Known_Candidate"), light green circles show SNR candidates newly identified here ("SMGPS_Candidate"), and yellow circles show “Unusual” sources ("SMGPS_Unusual"). Misidentified or nondetected SNRs and SNR candidates with dashed circles (filenames begin with "Bad"). Cyan scale bars at the lower left of each panel are 5' long.

SMGPS FITS files Stokes I SARAO MeerKAT Galactic Plane Survey (SMGPS) FITS cutouts for each SNR or SNR candidate. The data are from Goedhart et al., (2024). Each cutout has the source at the center of the field and dimensions of three times the source radius.

This data release was issued on 26 September 2024

Download	Description
Images	PDF images for each SNR or SNR candidate mentioned in the text. For each image, MIR data are in the left panels (Spitzer or WISE) and SMGPS 1.3 GHz data are on the right. White circles show HII regions from the WISE Catalog, blue-green circles show previously-known SNRs (filenames begin with "Known_Green" or "Known_SNRCat"), green circles show previously-known SNR candidates ("Known_Candidate"), light green circles show SNR candidates newly identified here ("SMGPS_Candidate"), and yellow circles show “Unusual” sources ("SMGPS_Unusual"). Misidentified or nondetected SNRs and SNR candidates with dashed circles (filenames begin with "Bad"). Cyan scale bars at the lower left of each panel are 5' long.
SMGPS FITS files	Stokes I SARAO MeerKAT Galactic Plane Survey (SMGPS) FITS cutouts for each SNR or SNR candidate. The data are from Goedhart et al., (2024). Each cutout has the source at the center of the field and dimensions of three times the source radius.