OAUNI photometry of SN 2023mkt
ATel #16234; A. Pereyra (Geophysical Institute of Peru, Astronomy Area), J. Tello (National University of Engineering - UNI, Peru), D. Alvarado (UNI), E. Torre (UNI), M. Zevallos (UNI), M. Espinoza (UNI), L. de Almeida (Universidade Federal do Rio Grande do Norte, Brasil)
on 7 Sep 2023; 15:10 UT
Credential Certification: Antonio Pereyra (apereyra@igp.gob.pe)
Subjects: Optical, Supernovae, Transient
We report photometry of Type Ia SN 2023mkt gathered with the OAUNI 51cm telescope at Huancayo Observatory, Peru. CCD imaging in R filter was performed on two consecutive nights under non-photometric conditions with an airmass lower than 1.7. The integration time was 90x20s=1800s in both nights. Our measurements are indicated below:
| Date (UT) |
filter |
seeing (") |
mag |
| 2023-08-18.082 |
R |
2.1 |
16.02 +/- 0.01 |
| 2023-08-19.079 |
R |
2.4 |
16.05 +/- 0.01 |
UCAC4 field stars were used for the zero point calibration. Our observations are ~6 weeks after SN 2023mkt discovery date. The OAUNI project is supported by UNI, TWAS, IGP and ProCiencia-Concytec (Convenio 133-2020 Fondecyt).
