OAUNI photometry of SN 2024jlf
| 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 | 2024-12-02T16:16:19Z | |
| dc.date.available | 2024-12-02T16:16:19Z | |
| dc.date.issued | 2024-11-25 | |
| dc.description.abstract | We report photometry of Type II SN 2024jlf 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 non-photometric conditions with airmasses lower than 1.3. The integration time was 40x20s=800s for all observations. Our measurements yielded: Date (UT) | filter | seeing (") | mag, 2024-06-05.056 | R | 2.5 | 14.71 +/- 0.01, 2024-06-06.024 | R | 2.7 | 14.57 +/- 0.03, 2024-06-07.013 | R | 2.9 | 14.45 +/- 0.03, 2024-06-08.010 | R | 2.7 | 14.54 +/- 0.02, 2024-06-09.005 | R | 2.5 | 14.66 +/- 0.02. UCAC4 field stars were used for the zero point calibration. Our first observation is ~8 days after ZTF discovery. 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/20.500.12816/5644 | |
| 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 2024jlf | |
| dc.type | info:eu-repo/semantics/report |