OAUNI photometry of SN 2023ixf
| dc.contributor.author | Pereyra, Antonio | |
| dc.contributor.author | Espinoza, M. | |
| dc.contributor.author | Tello, J. | |
| dc.contributor.author | Zevallos, M. | |
| dc.contributor.author | de Almeida, L. | |
| dc.contributor.author | Torre, E. | |
| dc.date.accessioned | 2023-07-04T22:44:03Z | |
| dc.date.available | 2023-07-04T22:44:03Z | |
| dc.date.issued | 2023-06-27 | |
| dc.description.abstract | We report photometry of Type II SN 2023ixf gathered with the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging in R filter was performed on two epochs under stable conditions (seeing ~1.7") and airmass lower than 2.5 (target with low altitude). Our integration times were 54x20s=1080s and 50x20s=1000s on 2023-06-20 and 2023-06-21, respectively. Our measurements yielded: on (UT) 2023-06-20.021, R = 11.28 +/- 0.02, and, on (UT) 2023-06-21.022, R = 11.30 +/- 0.02. UCAC4 field stars were used for the zero point calibration. Our observations are ~32-33 days after the earliest detection. | es_ES |
| dc.format | application/pdf | es_ES |
| dc.identifier.uri | http://hdl.handle.net/20.500.12816/5421 | |
| dc.language.iso | spa | es_ES |
| dc.publisher | Instituto Geofísico del Perú | 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 2023ixf | es_ES |
| dc.type | info:eu-repo/semantics/report | es_ES |