OAUNI photometry of SN2017gmr/DLT17cq

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).

Description

Date

2017-12-22

Keywords

Optical , Supernovae , Transient , Stars , Astronomical photometry , Supernova

Citation

URI

http://hdl.handle.net/20.500.12816/3317

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Files

ATel #11083.pdf (155.76 KB)

Authors

Pereyra, Antonio  
Ricra, J.

Publisher

The Astronomer's Telegram

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