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dc.date.accessioned 2019-12-03T14:58:02Z
dc.date.available 2019-12-03T14:58:02Z
dc.date.issued 2016
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/86651
dc.description.abstract We present a compilation of UBVRIz light curves of 51 type II supernovae discovered during the course of four different surveys during 1986-2003: the Cerro Tololo Supernova Survey, the Calán/Tololo Supernova Program (C&T), the Supernova Optical and Infrared Survey (SOIRS), and the Carnegie Type II Supernova Survey (CATS). The photometry is based on template-subtracted images to eliminate any potential host galaxy light contamination, and calibrated from foreground stars. This work presents these photometric data, studies the color evolution using different bands, and explores the relation between the magnitude at maximum brightness and the brightness decline parameter (s) from maximum light through the end of the recombination phase. This parameter is found to be shallower for redder bands and appears to have the best correlation in the B band. In addition, it also correlates with the plateau duration, being shorter (longer) for larger (smaller) s values. en
dc.language en es
dc.subject supernovae: general es
dc.subject surveys es
dc.subject techniques: photometric es
dc.title UBVRIz light curves of 51 type II supernovae en
dc.type Articulo es
sedici.identifier.other doi:10.3847/0004-6256/151/2/33 es
sedici.identifier.other eid:2-s2.0-84957954670 es
sedici.identifier.issn 0004-6256 es
sedici.creator.person Folatelli, Gastón es
sedici.description.note La lista completa de autores que integran el documento puede consultarse en el archivo. es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
mods.originInfo.place Instituto de Astrofísica de La Plata es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle The Astronomical Journal es
sedici.relation.journalVolumeAndIssue vol. 151, no. 2 es
sedici.rights.sherpa * Color: green * Pre-print del autor: can * Post-print del autor: can * Versión de editor/PDF:can * Condiciones: >>On any website, arXiv, scientific social networks (except Research Gate) or non-commercial open access repository. >>Publisher's version/PDF may be used on any website or authors' institutional repository >>Publisher copyright and source must be acknowledged >>Must link to publisher version >>Publisher's version/PDF may be used >>Authors depositing in arXiv must they choose the first licence statement offered by arXiv when uploading their article � a "non-exclusive licence to distribute" >>Publisher last contacted on 10/02/2016 >>Publisher last reviewed on 15/08/2017 * Link a Sherpa: http://sherpa.ac.uk/romeo/issn/0004-6256/es/


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)