OAUNI photometry of SN2017glq/Gaia17cfi

dc.contributor.authorPereyra, Antonio
dc.contributor.authorRicra, J.
dc.date.accessioned2018-11-06T12:10:45Z
dc.date.available2018-11-06T12:10:45Z
dc.date.issued2017-12-08
dc.description.abstractWe report optical photometry of Type Ia SN2017glq/Gaia17cfi (TNSDR 2017-13365, TNSCR 2017-1194) on 2017-09-19.182 (UT) gathered with the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging was performed using R band with seeing ~1.6" and airmass = 1.5. A total integration time of 59x20s=1180s yielded R = (14.16 +/- 0.05) mag. NOMAD field stars were used for the zero point calibration. Following OSC (Guillochon et al. 2016, arXiv:1605.01054) light curve, our measurements are very close to the 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/20.500.12816/3323
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.subjectAstronomical photometryes_ES
dc.subjectStarses_ES
dc.subjectSupernovaes_ES
dc.subject.ocdehttp://purl.org/pe-repo/ocde/ford#1.03.08es_ES
dc.titleOAUNI photometry of SN2017glq/Gaia17cfies_ES
dc.typeinfo:eu-repo/semantics/lecturees_ES

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