SN 2022bsi
SN 2022bsi was a Supernova Remnant. At 2022-02-28 04:04:10[1][2] Time in Moscow, Russia, a 25-year-old man discovered a Supernova[3] located in the galaxy NGC 5902. At UTC 2022-02-28 4:04, using a 15-meter-wide Palomar Telescope on February 9th, 2022, a Supernova candidate was identified using the CRTS (Carina Real-time Transient) and added to the Transient Name Server (TNS) as SN 2022bsi. It was also Filip Romanov's first supernovae discovery. Days later, using a remote telescope 21 located at the New Mexico Skies Observatory in Mayhill, New Mexico, the images were stacked, and it is currently classified as Ia-91bg, type Bg supernova.
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| Other designations | Lua error in Module:Wikidata at line 446: attempt to index field 'wikibase' (a nil value). |
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| Event type | lua error in module:wikidataib at line 665: attempt to index field 'wikibase' (a nil value). |
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| Epoch | J2000 |
| Galactic coordinates | 15h14m38.88s, +50°51′00.5 |
| Redshift | Lua error in Module:WikidataIB at line 665: attempt to index field 'wikibase' (a nil value). |
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| Preceded by | Lua error in Module:WikidataIB at line 665: attempt to index field 'wikibase' (a nil value). |
| Followed by | Lua error in Module:WikidataIB at line 665: attempt to index field 'wikibase' (a nil value). |
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References
- ↑ "Distant Supernova Discovered by Homeless Amateur Astronomer". MSN. Retrieved 2022-03-16.
- ↑ Fremling, C.; Romanov, F. (2022-02-01). "ZTF Transient Classification Report for 2022-02-28". Transient Name Server Classification Report. 2022-553: 1.
- ↑ Fremling, C.; Romanov, F. (2022-02-01). "ZTF Transient Classification Report for 2022-02-28". Transient Name Server Classification Report. 2022-553: 1.
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