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김재영

Kim, Jae-Young
Observational Astrophysics Lab
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EVN 5 GHz e-VLBI Observations of SN2023ixf in M101

Author(s)
Lee, DeokhyeongLee, Seung YeonParagi, ZsoltOrosz, GáborOh, JunghwanKim, Jae-Young
Issued Date
2024-05
DOI
10.3847/2515-5172/ad454e
URI
https://scholarworks.unist.ac.kr/handle/201301/83987
Citation
Research Notes of the American Astronomical Society, v.8, no.5, pp.121
Abstract
SN 2023ixf is a Type II-L supernova that occurred in M101 in 2023 May. The European VLBI Network (EVN) observed SN 2023ixf at 5 GHz approximately one month later, on June 28. We calibrated the EVN data using AIPS and CASA, reporting non-detection of a radio source with 5σ flux upper limits of 113 μJy and 135 μJy for both pipelines, respectively.
Publisher
IOP Publishing
ISSN
2515-5172

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