OAUNI photometry of ASASSN-16hz

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dc.contributor.authorPereyra, Antonio
dc.contributor.authorRicra, J.
dc.contributor.authorZevallos, M.
dc.date.accessioned2018-11-06T13:05:56Z
dc.date.available2018-11-06T13:05:56Z
dc.date.issued2016-12-07
dc.description.abstractWe report optical photometry of Type Ia SN ASASSN-16hz (=SN 2016eqb, ATel #9332, ATel #9333) on 2016-08-09 (UT) gathered with the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging was performed with seeing ~1.8" and airmass = 1.3. A total integration time of 900s (45x20s) and 880s (44x20s) in R and V filter, respectively, yielded: Date (UT) | filter | mag 2016-08-09.397 | R | 15.84 +/- 0.04 2016-08-09.412 | V | 15.82 +/- 0.05 UCAC4 field stars were used for the zero point calibration. Following Mayall/KOSMOS classification (ATel #9333), our measurements are ~2 days after maximum. The OAUNI project is supported by UNI, TWAS, IGP and Cienciactiva (Convenio 102-2015 Fondecyt)."es_ES
dc.formatapplication/pdfes_ES
dc.identifier.urihttp://hdl.handle.net/20.500.12816/3331
dc.language.isoenges_ES
dc.publisherThe Astronomer's Telegrames_ES
dc.rightsinfo:eu-repo/semantics/openAccesses_ES
dc.rights.urihttps://creativecommons.org/licences/by/4.0/es_ES
dc.subjectOpticales_ES
dc.subjectSupernovaees_ES
dc.subjectTransientes_ES
dc.subjectStarses_ES
dc.subjectSupernovaes_ES
dc.subjectAstronomical photometryes_ES
dc.subject.ocdehttp://purl.org/pe-repo/ocde/ford#1.03.08es_ES
dc.titleOAUNI photometry of ASASSN-16hzes_ES
dc.typeinfo:eu-repo/semantics/lecturees_ES

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