OAUNI photometry of SN 2023gfo

dc.contributor.authorPereyra, Antonio
dc.contributor.authorEspinoza, M.
dc.contributor.authorTello, J.
dc.contributor.authorZevallos, M.
dc.contributor.authorAlvarado, D.
dc.contributor.authorde Almeida, L.
dc.date.accessioned2023-06-14T16:34:44Z
dc.date.available2023-06-14T16:34:44Z
dc.date.issued2023-06-10
dc.description.abstractMultiband photometry of Type II SN 2023gfo on 2023-05-24 (UT) was gathered with the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging using VRI filters was performed under non-photometric conditions (seeing ~1.8") and airmass lower than 1.6. Total integration times of (45x20s=900s) for V, R and I filters yielded: V = 15.60 +/- 0.01 on 2023-05-24.228 (UT); R = 15.33 +/- 0.03 on 2023-05-24.197; I = 15.12 +/- 0.05 on 2023-05-24-212.es_ES
dc.formatapplication/pdfes_ES
dc.identifier.urihttp://hdl.handle.net/20.500.12816/5390
dc.language.isoenges_ES
dc.publisherR. E. Rutledgees_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 2023gfoes_ES
dc.typeinfo:eu-repo/semantics/reportes_ES

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