OAUNI photometry of SN 2023mkt

• Autores: Pereyra, Antonio, Tello, J., Alvarado, D., Torre, E., Zevallos, M., de Almeida, L.
• Formato: informe técnico
• Fecha de Publicación: 2023
• Institución: Instituto Geofísico del Perú
• Repositorio: IGP-Institucional
• Lenguaje: inglés
• OAI Identifier: oai:repositorio.igp.gob.pe:20.500.12816/5492
• Enlace del recurso: http://hdl.handle.net/20.500.12816/5492
• Nivel de acceso: acceso abierto
• Materia: Optical; Supernovae; Transient; http://purl.org/pe-repo/ocde/ford#1.03.08

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).