6.1 Proyectos de investigación científica
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PublicaciónOAUNI photometry of ASASSN-16gq/AT2016cym(The Astronomer's Telegram, 2017-04-21)
;Pereyra, Antonio ;Ricra, J.Zevallos, M.We report optical photometry of Type Ia SN ASASSN-16gq/AT2016cym (ATel #9199, ATel #9219) on 2016-07-11 (UT) gathered with the OAUNI 51cm telescope at Huancayo Observatory, Peru. -
PublicaciónOAUNI photometry of ASASSN-16hz(The Astronomer's Telegram, 2016-12-07)
;Pereyra, Antonio ;Ricra, J.Zevallos, M.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) -
PublicaciónOAUNI photometry of SN2017gmr/DLT17cq(The Astronomer's Telegram, 2017-12-22)
;Pereyra, AntonioRicra, J.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).