OAUNI optical observation of the supernova ASASSN-15lp

Descripción del Articulo

During the commissioning runs of the National University of Engineering's Astronomical Observatory (OAUNI) project, we report optical imaging of the Type Ia SN ASASSN-15lp (ATel #7691, ATel #7692) on 2015-07-17.352 (UT). The measurement was gathered using the OAUNI 51cm telescope at the Huancay...

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Detalles Bibliográficos
Autores: Pereyra, Antonio, Cori, W., Meza, E., Ricra, J., Zevallos, M.
Formato: ponencia
Fecha de Publicación:2015
Institución:Instituto Geofísico del Perú
Repositorio:IGP-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.igp.gob.pe:20.500.12816/3338
Enlace del recurso:http://hdl.handle.net/20.500.12816/3338
Nivel de acceso:acceso abierto
Materia:Optical
Supernovae
Stars
Supernova
Astronomical photometry
http://purl.org/pe-repo/ocde/ford#1.03.08
Descripción
Sumario:During the commissioning runs of the National University of Engineering's Astronomical Observatory (OAUNI) project, we report optical imaging of the Type Ia SN ASASSN-15lp (ATel #7691, ATel #7692) on 2015-07-17.352 (UT). The measurement was gathered using the OAUNI 51cm telescope at the Huancayo Observatory, Peru (3300 masl at the central peruvian Andes). The observation was made under non-photometric clear skies and through an airmass of 1.4. A 180-second exposure in V filter yielded V = (15.86 +/- 0.05) mag. The zero point calibration was obtained using comparison stars in the neighborhood of the field. Our measurement is 28 days after the discovery (ATel #7691) and caution must be taken for contamination with the host galaxy. The OAUNI project is supported by UNI, The World Academy of Sciences (TWAS) and IGP.
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