E5: Evolution, Energetics and Environments of Extreme Explosions

Logo copyright © Poonam Chandra

GLIMPSE: GMRT Low-frequency Imaging to unveil the Massive Progenitors of Supernovae Explosions

This survey is part of the larger project: "E5: Evolution, Energetics and Environments of Extreme Explosions", © Poonam Chandra.

Light curves are provided for detections at multiple epochs.

e
Supernova Type Redshift GMRT Bands ☨ Detected
SN 2023ixf * II 0.000804 Bands 5, 4 No
SN 2023gfo * II 0.006 Bands 5 No
SN 2023esp II 0.008 Bands 5 No
SN 2023axu II - Bands 5 No
SN 2022acko II 0.005264 Bands 5 No
SN 2022xxf * Ic-BL 0.0053 Bands 5, 4 Light Curve
SN 2022qhy Ibn 0.006124 Bands 5 No
SN 2022crv * Ib/IIb 0.008091 Bands 5, 4, 3 Light Curve
SN 2021afug Bands 5 No
SN 2021yja IIP 0.0053 Bands 5, 4 Light Curve
SN 2021uha Bands 5 No
SN 2021csp Bands 5 No
SN 2021bhd Bands 5 and 4 No
SN 2020adow Bands 5 No
SN 2020acat IIb 0.0079 Bands 5, 4 Light Curve
SN 2020ywx * IIn 0.0217 Bands 5, 4, 3 Light Curve
SN 2020uem Bands 5 No
SN 2020qmp Bands 5 and 4 No
SN 2020ocz Bands 5 No
SN 2020jfo Bands 5 No
SN 2020bvc Ic-BL 0.025235 Bands 5, 4 Light Curve
SN 2020bio Bands 5 and 4 No
SN 2020vg Bands 5 No
SN 2020oi Bands 5 and 4 No
SN 2020ad Bands 5 and 4 Light Curve
SN 2019yvr * Ib 0.005 Bands 5, 4, 3 Light Curve
SN 2019xhb Bands 5 and 4 Light Curve
SN 2019vxm Bands 5 and 4 No
SN 2019muj Bands 5 No

☨ The uGMRT bands are: Band 5 (1000-1450 MHz), Band 4 (550-900 MHz), Band 3 (250-500 MHz)
Supernovae with * symbols are being actively followed up with the uGMRT.