OAUNI photometry of SN2022jli
| dc.contributor.author | Pereyra, Antonio | |
| dc.contributor.author | Tello, J. | |
| dc.contributor.author | Zevallos, M. | |
| dc.contributor.author | de Almeida, L. | |
| dc.contributor.author | Espinoza, M. | |
| dc.contributor.author | Alvarado, D. | |
| dc.date.accessioned | 2022-09-19T12:40:23Z | |
| dc.date.available | 2022-09-19T12:40:23Z | |
| dc.date.issued | 2022-07-24 | |
| dc.description.abstract | Multiband photometry of Type Ic SN2022jli (TNSTR-2022-1198, TNSCR-2022-1261) on 2022-07-01 (UT) was gathered with the OAUNI 51cm telescope (arXiv:1512.03104) at Huancayo Observatory, Peru. CCD imaging using VRI filters was performed under non-photometric conditions (seeing ~2.3") and airmass lower than 1.3. Total integration times of (60x20s=1200s) for V, R and I filters yielded: Date (UT) filter mag 2022-07-01.401 V 14.64 +/- 0.04 2022-07-01.359 R 14.52 +/- 0.05 2022-07-01.381 I 14.06 +/- 0.05. UCAC4 field stars were used for the zero point calibration. Caution must be taken in SN2022jli magnitudes for possible contamination with the host galaxy. Following GELATO and SNID classification (TNSCR-2022-1261), our measurements are aprox. 52 days after maximum brightness. The OAUNI project is supported by UNI, TWAS, IGP and ProCiencia-Concytec (Convenio 133-2020 Fondecyt). | es_ES |
| dc.format | application/pdf | es_ES |
| dc.identifier.uri | http://hdl.handle.net/20.500.12816/5282 | |
| dc.language.iso | spa | es_ES |
| dc.publisher | R. E. Rutledge | es_ES |
| dc.rights | info:eu-repo/semantics/openAccess | es_ES |
| dc.rights.uri | https://creativecommons.org/licenses/by-nc-nd/4.0/ | es_ES |
| dc.subject | Optical | es_ES |
| dc.subject | Supernovae | es_ES |
| dc.subject | Astronomy | es_ES |
| dc.subject.ocde | http://purl.org/pe-repo/ocde/ford#1.03.08 | es_ES |
| dc.title | OAUNI photometry of SN2022jli | es_ES |
| dc.type | info:eu-repo/semantics/report | es_ES |