AstroNote 2024-134

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DRAFT
2024-05-23 14:39:43
Type: Object/s-Data/Analysis
AMI-LA radio detection of the type II SN 2024iss
Authors: Itai Sfaradi (HUJI), Assaf Horesh (HUJI), Lauren Rhodes (Oxford), Rob Fender (Oxford), Joe Bright (Oxford), Dave Green (Cambridge), David Titterington (Cambridge)
Keywords: Radio, Supernova

We observed the field of the type II SN 2024iss (TNS report 210230) with the Arcminute Microkelvin Imager - Large Array (AMI-LA) for 4 hours on the 2024-05-22, with a central frequency of 15.5 GHz. A point source is detected in the AMI-LA image at RA = 12:59:06.089 +/- 0.01 s, Dec = +28:48:41.16 +/- 1.87 arcsec, consistent with the reported position of SN 2024iss. The source is detected at a flux density of 3.5 +/- 0.2 mJy.

Past pre-discovery radio observation of the field of SN 2024iss was performed by the VLA Sky Survey (VLASS) on 2023-01-18 (epoch 3.1), at a central frequency of 3 GHz. The VLASS image of the field of SN 2024iss shows no emission from the reported position with a 3-sigma rms of 0.35 mJy.

We plan to perform follow-up observations with the AMI-LA and encourage further high-cadence multi-frequency radio observations with other facilities.

We thank the staff of MRAO for scheduling and performing this observation.

Show current TNS values
CatalogNameReported RAReported DECReported Obj-TypeReported RedshiftHost NameHost RedshiftRemarksTNS RATNS DECTNS Obj-TypeTNS Redshift
TNS2024iss12:59:06.145+28:48:42.67SN II0.0033312:59:06.130+28:48:42.62SN IIb0.003334