OAUNI photometry of ASASSN-16hw

dc.contributor.authorPereyra, Antonio
dc.contributor.authorRicra, J.
dc.contributor.authorZevallos, M.
dc.date.accessioned2018-11-06T13:13:34Z
dc.date.available2018-11-06T13:13:34Z
dc.date.issued2016-09-30
dc.description.abstractWe report optical photometry of Type Ia SN ASASSN-16hw (=SN 2016ekt, ATel #9278, ATel #9289, ATel #9300) on 2016-08-06 (UT) gathered with the OAUNI 51cm telescope (Pereyra et al. 2015;arXiv:1512.03104) at Huancayo Observatory, Peru. CCD imaging measurements using V and R broadband filters were acquired with seeing ~1.9" and airmass = 1.5. A total integration time of 42x20s=840s in each filter yielded: Date (UT) filter mag 2016-08-06.119 R 14.656 +/- 0.003 2016-08-06.120 V 14.497 +/- 0.004 Field stars were used for the zero point calibration. Following PESSTO and Du Pont classifications (ATel #9289, ATel #9300), our measurements are very close to 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/20.500.12816/3333
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.subjectAstronomical photometryes_ES
dc.subjectSupernovaes_ES
dc.subject.ocdehttp://purl.org/pe-repo/ocde/ford#1.03.08es_ES
dc.titleOAUNI photometry of ASASSN-16hwes_ES
dc.typeinfo:eu-repo/semantics/lecturees_ES

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