Publicación:
OAUNI photometry of SN2017gmr/DLT17cq
OAUNI photometry of SN2017gmr/DLT17cq
| dc.contributor.author | Pereyra, Antonio | es_PE |
| dc.contributor.author | Ricra, J. | es_PE |
| dc.date.accessioned | 2024-05-30T23:13:38Z | |
| dc.date.available | 2024-05-30T23:13:38Z | |
| dc.date.issued | 2017-12-22 | |
| 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). | |
| dc.description.sponsorship | Consejo Nacional de Ciencia, Tecnología e Innovación Tecnológica - Concytec | |
| dc.identifier.uri | https://hdl.handle.net/20.500.12390/828 | |
| dc.language.iso | eng | |
| dc.publisher | The Astronomer's Telegram | |
| dc.rights | info:eu-repo/semantics/openAccess | |
| dc.rights.uri | https://creativecommons.org/licenses/by-nc-nd/4.0/ | |
| dc.subject | Supernova | |
| dc.subject | Estrellas | es_PE |
| dc.subject | Fotometría astronómica | es_PE |
| dc.subject | Óptica | es_PE |
| dc.subject | info:eu-repo/semantics/lecture | es_PE |
| dc.subject.ocde | http://purl.org/pe-repo/ocde/ford#1.03.08 | |
| dc.title | OAUNI photometry of SN2017gmr/DLT17cq | |
| dc.type | info:eu-repo/semantics/lecture | |
| dspace.entity.type | Publication |