| dc.creator | Pereyra, Antonio | |
| dc.creator | Ricra, J. | |
| dc.creator | Zevallos, M. | |
| dc.date.accessioned | 2018-11-06T13:05:56Z | |
| dc.date.accessioned | 2023-05-24T14:22:38Z | |
| dc.date.available | 2018-11-06T13:05:56Z | |
| dc.date.available | 2023-05-24T14:22:38Z | |
| dc.date.created | 2018-11-06T13:05:56Z | |
| dc.date.issued | 2016-12-07 | |
| dc.identifier | http://hdl.handle.net/20.500.12816/3331 | |
| dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/6428997 | |
| 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) | filter | mag 2016-08-09.397 | R | 15.84 +/- 0.04 2016-08-09.412 | V | 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.language | eng | |
| dc.publisher | The Astronomer's Telegram | |
| dc.rights | https://creativecommons.org/licences/by/4.0/ | |
| dc.rights | info:eu-repo/semantics/openAccess | |
| dc.subject | Optical | |
| dc.subject | Supernovae | |
| dc.subject | Transient | |
| dc.subject | Stars | |
| dc.subject | Supernova | |
| dc.subject | Astronomical photometry | |
| dc.title | OAUNI photometry of ASASSN-16hz | |
| dc.type | info:eu-repo/semantics/lecture | |
