OAUNI photometry of SN 2023ixf

dc.contributor.authorPereyra, Antonio
dc.contributor.authorEspinoza, M.
dc.contributor.authorTello, J.
dc.contributor.authorZevallos, M.
dc.contributor.authorde Almeida, L.
dc.contributor.authorTorre, E.
dc.date.accessioned2023-07-04T22:44:03Z
dc.date.available2023-07-04T22:44:03Z
dc.date.issued2023-06-27
dc.description.abstractWe 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.formatapplication/pdfes_ES
dc.identifier.urihttp://hdl.handle.net/20.500.12816/5421
dc.language.isospaes_ES
dc.publisherInstituto GeofĂ­sico del PerĂșes_ES
dc.rightsinfo:eu-repo/semantics/openAccesses_ES
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/es_ES
dc.subjectOpticales_ES
dc.subjectSupernovaees_ES
dc.subjectTransientes_ES
dc.subject.ocdehttp://purl.org/pe-repo/ocde/ford#1.03.08es_ES
dc.titleOAUNI photometry of SN 2023ixfes_ES
dc.typeinfo:eu-repo/semantics/reportes_ES

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