OAUNI photometry of SN 2023mkt

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dc.contributor.authorPereyra, Antonio
dc.contributor.authorTello, J.
dc.contributor.authorAlvarado, D.
dc.contributor.authorTorre, E.
dc.contributor.authorZevallos, M.
dc.contributor.authorde Almeida, L.
dc.date.accessioned2023-11-27T19:00:54Z
dc.date.available2023-11-27T19:00:54Z
dc.date.issued2023-09-07
dc.description.abstractWe 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.formatapplication/pdfes_ES
dc.identifier.urihttp://hdl.handle.net/20.500.12816/5492
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 2023mktes_ES
dc.typeinfo:eu-repo/semantics/reportes_ES

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