OAUNI photometry of SN 2024ggi
| dc.contributor.author | Pereyra, Antonio | |
| dc.contributor.author | Zevallos, M. | |
| dc.contributor.author | Alvarado, D. | |
| dc.contributor.author | Delgado, J. | |
| dc.contributor.author | Tello, J. | |
| dc.contributor.author | de Almeida, L. | |
| dc.contributor.author | Torre, E. | |
| dc.date.accessioned | 2024-12-02T16:15:54Z | |
| dc.date.available | 2024-12-02T16:15:54Z | |
| dc.date.issued | 2024-11-25 | |
| dc.description.abstract | We report photometry of Type II SN 2024ggi gathered with the OAUNI 51cm telescope (arXiv:1512.03104) at Huancayo Observatory, Peru. CCD imaging in R filter was performed on five consecutive nights under nonˇphotometric conditions with airmasses lower than 1.6. The integration time was 50x20s=1000s in the first observation and 60x20s=1200s for the rest. Our measurements yielded: Date (UT) | filter | seeing (") | mag, 2024-06-05.108 | R | 3.2 | 12.27 +/- 0.06, 2024-06-06.080 | R | 2.6 | 12.25 +/- 0.06, 2024-06-07.064 | R | 2.8 | 12.27 +/- 0.06, 2024-06-08.061 | R | 2.7 | 12.27 +/- 0.06, 2024-06-09.062 | R | 2.9 | 12.28 +/- 0.06. UCAC4 field stars were used for the zero point calibration. Our observations are ~7.9 weeks after ATLAS discovery (TNSAN-2024-100). The OAUNI project is supported by UNI, TWAS, IGP and ProCiencia-Concytec (Convenio 133-2020 Fondecyt). | |
| dc.description.sponsorship | El proyecto OAUNI cuenta con el apoyo de UNI, TWAS, IGP y ProCiencia-Concytec [Convenio 133-2020 Fondecyt]. | |
| dc.format | application/pdf | |
| dc.identifier.uri | http://hdl.handle.net/20.500.12816/5643 | |
| dc.language.iso | eng | |
| dc.publisher | R. E. Rutledge | |
| dc.rights | info:eu-repo/semantics/openAccess | |
| dc.rights.uri | https://creativecommons.org/licenses/by/4.0/ | |
| dc.subject | Optical | |
| dc.subject | Supernovae | |
| dc.subject | Transient | |
| dc.subject.ocde | https://purl.org/pe-repo/ocde/ford#1.03.08 | |
| dc.title | OAUNI photometry of SN 2024ggi | |
| dc.type | info:eu-repo/semantics/report |