OAUNI photometry of ASASSN-16gq/AT2016cym

dc.contributor.authorPereyra, Antonio
dc.contributor.authorRicra, J.
dc.contributor.authorZevallos, M.
dc.date.accessioned2018-11-06T12:47:21Z
dc.date.available2018-11-06T12:47:21Z
dc.date.issued2017-04-21
dc.description.abstractWe report optical photometry of Type Ia SN ASASSN-16gq/AT2016cym (ATel #9199, ATel #9219) on 2016-07-11 (UT) gathered with the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging was performed with seeing ~1.7" and airmass = 1.3. Our measurements yielded: Date (UT) | filter | IT | mag 2016-07-11.085 | V | 1200s (60x20s) | 17.94 +/- 0.06 2016-07-11.106 | R | 0760s (38x20s) | 17.84 +/- 0.04 Field stars were used for the zero point calibration. Caution must be taken for contamination of edge-on Sc host galaxy (ESO 446-G023). Following FLWO/FAST classification (ATel #9219), our measurements are ~17 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/20.500.12816/3327
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-16gq/AT2016cymes_ES
dc.typeinfo:eu-repo/semantics/lecturees_ES

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