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V band photometry of the SN 2003GF supernova utilizing the 2mass catalog

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dc.contributor.author Reyes, RC es_PE
dc.contributor.author Ferrero, G es_PE
dc.contributor.author Navarro, FAR es_PE
dc.contributor.author Melendez, J es_PE
dc.date.accessioned 2024-05-30T23:13:38Z
dc.date.available 2024-05-30T23:13:38Z
dc.date.issued 2013
dc.description This research was carried out as part of the project titled "Variabilidad Estelar en la Galaxia" (Stellar Variability in the Galaxy) supported by CONCYTEC (Consejo Nacional de Ciencia, Tecnologia e Innovacion Tecnologica, Peru). We also thank the 2MASS, SIMBAD, ALADIN, and VSNET online databases which allowed us access to valuable data from other observers.
dc.description.abstract We obtained several images of SN 2003gf at the Marangani Observatory (Peru) on the night 3–4 July 2003 from which we have estimated its brightnessin the V band, as 15.10 ± 0.09 mag. This was obtained after a proper calibration of the starfield, considering the photometric data of the infrared bands of the 2MASScatalog. The precision achieved shows a reasonable agreement with measurements by other observers
dc.description.sponsorship Consejo Nacional de Ciencia, Tecnología e Innovación Tecnológica - Concytec
dc.identifier.isi 325508100016
dc.identifier.uri https://hdl.handle.net/20.500.12390/1123
dc.language.iso eng
dc.publisher Revista Mexicana de Astronomıa y Astrofisica
dc.relation.ispartof Revista Mexicana de Astronomía y Astrofísica
dc.rights info:eu-repo/semantics/openAccess
dc.subject Telescopios
dc.subject Supernovas es_PE
dc.subject Fotométricas es_PE
dc.subject.ocde https://purl.org/pe-repo/ocde/ford#1.03.08
dc.title V band photometry of the SN 2003GF supernova utilizing the 2mass catalog
dc.type info:eu-repo/semantics/article
dspace.entity.type Publication
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