OAUNI photometry of SN2017glq/Gaia17cfi
| 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.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.identifier.uri | http://hdl.handle.net/20.500.12816/3323 | |
| 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.subject.ocde | http://purl.org/pe-repo/ocde/ford#1.03.08 | es_ES |
| dc.title | OAUNI photometry of SN2017glq/Gaia17cfi | es_ES |
| dc.type | info:eu-repo/semantics/lecture | es_ES |