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dc.contributor.authorGalbany, L.-
dc.contributor.authorPérez Jiménez, Enrique-
dc.contributor.authorMoral, V.-
dc.date.accessioned2017-05-24T11:50:55Z-
dc.date.available2017-05-24T11:50:55Z-
dc.date.issued2016-
dc.identifierdoi: 10.1093/mnras/stv2620-
dc.identifierissn: 1365-2966-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society 455: 4087- 4099 (2016)-
dc.identifier.urihttp://hdl.handle.net/10261/150282-
dc.description.abstractWe present a statistical analysis of the environments of 11 supernovae (SNe) which occurred in six nearby galaxies (z ≲ 0.016). All galaxies were observed with MUSE, the high spatial resolution integral-field spectrograph mounted to the 8 m VLT UT4. These data enable us to map the full spatial extent of host galaxies up to ~3 effective radii. In this way, not only can one characterize the specific host environment of each SN, one can compare their properties with stellar populations within the full range of other environments within the host. We present a method that consists of selecting all HII regions found within host galaxies from 2D extinction-corrected Hα emission maps. These regions are then characterized in terms of their Hα equivalent widths, star formation rates and oxygen abundances. Identifying HII regions spatially coincident with SN explosion sites, we are thus able to determine where within the distributions of host galaxy e.g. metallicities and ages each SN is found, thus providing new constraints on SN progenitor properties. This initial pilot study using MUSE opens the way for a revolution in SN environment studies where we are now able to study multiple environment SN progenitor dependencies using a single instrument and single pointing. © 2015 The Authors.-
dc.description.sponsorshipSupport for LG, HK, MH, SGG and FF is provided by the Ministry of Economy, Development, and Tourism's Millennium Science Initiative through grant IC120009, awarded to The Millennium Institute of Astrophysics, MAS. LG, HK and FF acknowledge support by CONICYT through FONDECYT grants 3140566, 3140563 and 11130228, respectively. EP acknowledges support from Spanish MINECO project AYA2014-57490P and Junta de Andalucia FQ1580.-
dc.publisherOxford University Press-
dc.relationMINECO/ICTI2013-2016/AYA2014-57490P-
dc.relation.isversionofPublisher's version-
dc.rightsopenAccess-
dc.subjectSupernovae: general-
dc.subjectTechniques: spectroscopic-
dc.subjectMethods: statistical-
dc.subjectH II regions-
dc.subjectGalaxies: general-
dc.titleCharacterizing the environments of supernovae with MUSE-
dc.typeArtículo-
dc.identifier.doi10.1093/mnras/stv2620-
dc.date.updated2017-05-24T11:50:55Z-
dc.description.versionPeer Reviewed-
dc.language.rfc3066eng-
dc.rights.licensehttp://dx.doi.org/10.1093/mnras/stv2620-
dc.contributor.funderComisión Nacional de Investigación Científica y Tecnológica (Chile)-
dc.contributor.funderMinisterio de Economía y Competitividad (España)-
dc.contributor.funderJunta de Andalucía-
dc.contributor.funderMinisterio de Economía, Fomento y Turismo (Chile)-
dc.relation.csic-
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003329es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100005886es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100002848es_ES
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