DRAFT
2023-05-27 00:05:53
Type: Object/s-Data/Analysis
Bibcode: 2023TNSAN.146....1M
VLA 10 GHz Observations of SN2023ixf
Authors: David Matthews, Raffaella Margutti (UC Berkeley), Kate D. Alexander (University of Arizona), Joe Bright (University of Oxford), Yvette Cendes, Edo Berger (Center for Astrophysics | Harvard & Smithsonian), Tanmoy Lasker (University of Utah), Maria Drout (University of Toronto), Danny Milisavljevic (Purdue University)
Keywords: Supernova, Radio, Transient
Abstract:
We report the radio non-detection of SN2023ixf in the nearby galaxy M101 at 10 GHz.

We report radio observations of SN2023ixf with NSF’s Karl G. Jansky Very Large Array (VLA). We observed SN2023ixf with the VLA on May 23rd 2023 beginning on-source at 00:24:09 UT (~4 days since discovery, Project Code SF151070, PI: Margutti) at X-band (8-12 GHz) with the array in B-configuration for a duration of approximately 40 minutes. We find no evidence for statistically significant radio emission at the location of SN2023ixf with a preliminary 5x RMS upper limit of 33 uJy.

Further observations are planned.

We thank the entire VLA team for carrying out these observations.

Show current TNS values
Catalog Name Reported RA Reported DEC Reported Obj-Type Reported Redshift Host Name Host Redshift Remarks TNS RA TNS DEC TNS Obj-Type TNS Redshift
TNS 2023ixf [ZTF23aaklqou] 14:03:38.562 +54:18:41.94 SN IIn 0.0008 M101 14:03:38.562 +54:18:41.94 SN II 0.0008

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