OAUNI photometry of ASASSN-16hz Pereyra, Antonio es_PE Ricra, J. es_PE Zevallos, M. es_PE 2024-05-30T23:13:38Z 2024-05-30T23:13:38Z 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.language.iso eng
dc.publisher The Astronomer's Telegram
dc.rights info:eu-repo/semantics/openAccess
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.title OAUNI photometry of ASASSN-16hz
dc.type info:eu-repo/semantics/lecture
dspace.entity.type Publication