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dc.contributor.author Pereyra, Antonio
dc.contributor.author Ricra, J.
dc.date.accessioned 2018-11-06T11:21:49Z
dc.date.available 2018-11-06T11:21:49Z
dc.date.issued 2017-12-22
dc.identifier.uri http://hdl.handle.net/20.500.12816/3317
dc.description.abstract Optical photometry of Type II SN2017gmr/DLT17cq (ATel #10706, ATel #10717, TNSCR 2017-1220) on 2017-09-19.207 (UT) was gathered using the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging was performed in R band with seeing ~1.5" and airmass = 1.3. A total integration time of 55x20s=1100s yielded R = (14.05 +/- 0.04) mag. NOMAD field stars were used for the zero point calibration. 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 Stars es_ES
dc.subject Astronomical photometry es_ES
dc.subject Supernova es_ES
dc.title OAUNI photometry of SN2017gmr/DLT17cq 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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