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- Kim, Jae-Young
- Observational Astrophysics Lab
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| DC Field | Value | Language |
|---|---|---|
| dc.citation.number | 5 | - |
| dc.citation.startPage | 121 | - |
| dc.citation.title | Research Notes of the American Astronomical Society | - |
| dc.citation.volume | 8 | - |
| dc.contributor.author | Lee, Deokhyeong | - |
| dc.contributor.author | Lee, Seung Yeon | - |
| dc.contributor.author | Paragi, Zsolt | - |
| dc.contributor.author | Orosz, Gábor | - |
| dc.contributor.author | Oh, Junghwan | - |
| dc.contributor.author | Kim, Jae-Young | - |
| dc.date.accessioned | 2024-10-02T14:05:05Z | - |
| dc.date.available | 2024-10-02T14:05:05Z | - |
| dc.date.created | 2024-10-02 | - |
| dc.date.issued | 2024-05 | - |
| dc.description.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. | - |
| dc.identifier.bibliographicCitation | Research Notes of the American Astronomical Society, v.8, no.5, pp.121 | - |
| dc.identifier.doi | 10.3847/2515-5172/ad454e | - |
| dc.identifier.issn | 2515-5172 | - |
| dc.identifier.uri | https://scholarworks.unist.ac.kr/handle/201301/83987 | - |
| dc.language | 영어 | - |
| dc.publisher | IOP Publishing | - |
| dc.title | EVN 5 GHz e-VLBI Observations of SN2023ixf in M101 | - |
| dc.type | Article | - |
| dc.description.isOpenAccess | TRUE | - |
| dc.type.docType | Article | - |
| dc.description.journalRegisteredClass | foreign | - |
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