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dc.contributor.author Pereyra, Antonio
dc.contributor.author Ricra, J.
dc.date.accessioned 2018-11-06T12:10:45Z
dc.date.available 2018-11-06T12:10:45Z
dc.date.issued 2017-12-08
dc.identifier.uri http://hdl.handle.net/20.500.12816/3323
dc.description.abstract We 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.format application/pdf es_ES
dc.language.iso eng es_ES
dc.publisher The Astronomer's Telegram es_ES
dc.rights info:eu-repo/semantics/openAccess es_ES
dc.rights.uri https://creativecommons.org/licences/by/4.0/ es_ES
dc.subject Optical es_ES
dc.subject Supernovae es_ES
dc.subject Transient es_ES
dc.subject Astronomical photometry es_ES
dc.subject Stars es_ES
dc.subject Supernova es_ES
dc.title OAUNI photometry of SN2017glq/Gaia17cfi es_ES
dc.type info:eu-repo/semantics/lecture es_ES
dc.subject.ocde http://purl.org/pe-repo/ocde/ford#1.03.08 es_ES

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