OAUNI photometry of SN 2023mkt
| dc.contributor.author | Pereyra, Antonio | |
| dc.contributor.author | Tello, J. | |
| dc.contributor.author | Alvarado, D. | |
| dc.contributor.author | Torre, E. | |
| dc.contributor.author | Zevallos, M. | |
| dc.contributor.author | de Almeida, L. | |
| dc.date.accessioned | 2023-11-27T19:00:54Z | |
| dc.date.available | 2023-11-27T19:00:54Z | |
| dc.date.issued | 2023-09-07 | |
| dc.description.abstract | We report photometry of Type Ia SN 2023mkt gathered with the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging in R filter was performed on two consecutive nights under non-photometric conditions with an airmass lower than 1.7. The integration time was 90x20s=1800s in both nights. Our measurements are indicated below: Date (UT) | filter |seeing (") | mag, 2023-08-18.082 | R | 2.1 | 16.02 +/- 0.01, 2023-08-19.079 | R | 2.4 |16.05 +/- 0.01. UCAC4 field stars were used for the zero point calibration. Our observations are ~6 weeks after SN 2023mkt discovery date. 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/20.500.12816/5492 | |
| dc.language.iso | eng | 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 | Transient | es_ES |
| dc.subject.ocde | http://purl.org/pe-repo/ocde/ford#1.03.08 | es_ES |
| dc.title | OAUNI photometry of SN 2023mkt | es_ES |
| dc.type | info:eu-repo/semantics/report | es_ES |