OAUNI photometry of SN 2023ijd
| 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 | Alvarado, D. | |
| dc.date.accessioned | 2023-09-22T15:54:21Z | |
| dc.date.available | 2023-09-22T15:54:21Z | |
| dc.date.issued | 2023-07-31 | |
| dc.description.abstract | Photometry of Type II SN 2023ijd (TNSTR-2023-1092, TNSCR-2023-1112) was gathered with the OAUNI 51cm telescope (arXiv:1512.03104) at Huancayo Observatory, Peru. CCD imaging in R filter was performed on three consecutive nights under non-photometric conditions with airmasses lower than 1.8. The integration time was 70x20s=1400s in each observation. Our measurements yielded: Date (UT) / filter / seeing (") / mag ; 2023-07-15.072 / R / 2.1 / 15.52 +/- 0.01 ; 2023-07-16.057 / R / 1.8 / 15.61 +/- 0.01 ; 2023-07-17.053 / R / 2.2 / 15.56 +/- 0.01. UCAC4 field stars were used for the zero point calibration. Our observations are ~two months after the ASAS-SN detection (TNSTR-2023-1092). 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/20.500.12816/5462 | |
| 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 2023ijd | es_ES |
| dc.type | info:eu-repo/semantics/report | es_ES |