Erratum: Flux density uncertainties for SN 2022crv in ATel 15257
ATel #15260; S. D. Ryder (Macquarie University), L. Marnoch (Macquarie University), E. Kundu (Michigan State University), M. D. Filipovic (Western Sydney University), R. Z. E. Alsaberi (Western Sydney University), G. Anderson (ICRAR/Curtin University), C. Stockdale (Marquette University), K. Maeda (Kyoto University), M. Renaud (LUPM, CNRS/IN2P3), R. Kotak (University of Turku)
on 3 Mar 2022; 22:12 UT
Credential Certification: Stuart Ryder (Stuart.Ryder@mq.edu.au)
Subjects: Radio, Supernovae
In ATel #15257 we reported the radio detection of SN 2022crv, but omitted to include uncertainties on the flux densities. The measured flux densities of SN 2022crv on 1 March 2022 UT were 0.50 +/- 0.05 mJy at 5.5 GHz, and 0.75 +/- 0.09 mJy at 9.0 GHz. We apologise for the oversight. Further radio observations are planned in the coming weeks, and multi-wavelength follow-up is encouraged.
