Publicación:
OAUNI photometry of ASASSN-16hz
OAUNI photometry of ASASSN-16hz
| dc.contributor.author | Pereyra, Antonio | es_PE |
| dc.contributor.author | Ricra, J. | es_PE |
| dc.contributor.author | Zevallos, M. | es_PE |
| dc.date.accessioned | 2024-05-30T23:13:38Z | |
| dc.date.available | 2024-05-30T23:13:38Z | |
| dc.date.issued | 2016-12-07 | |
| dc.description.abstract | We report optical photometry of Type Ia SN ASASSN-16hz (=SN 2016eqb, ATel #9332, ATel #9333) on 2016-08-09 (UT) gathered with the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging was performed with seeing ~1.8" and airmass = 1.3. A total integration time of 900s (45x20s) and 880s (44x20s) in R and V filter, respectively, yielded: Date (UT) | |
| dc.description.abstract | filter | |
| dc.description.abstract | mag 2016-08-09.397 | |
| dc.description.abstract | R | |
| dc.description.abstract | 15.84 +/- 0.04 2016-08-09.412 | |
| dc.description.abstract | V | |
| dc.description.abstract | 15.82 +/- 0.05 UCAC4 field stars were used for the zero point calibration. Following Mayall/KOSMOS classification (ATel #9333), our measurements are ~2 days after maximum. 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/20.500.12390/830 | |
| 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 | https://purl.org/pe-repo/ocde/ford#1.03.08 | |
| dc.title | OAUNI photometry of ASASSN-16hz | |
| dc.type | info:eu-repo/semantics/lecture | |
| dspace.entity.type | Publication |