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Authordc.contributor.authorKrisciunas, Kevin 
Authordc.contributor.authorSuntzeff, Nicholas B. es_CL
Authordc.contributor.authorPhillips, Mark M. es_CL
Authordc.contributor.authorCandia, Pablo es_CL
Authordc.contributor.authorPrieto, José Luis es_CL
Authordc.contributor.authorAntezana, Roberto es_CL
Authordc.contributor.authorChassagne, Robin es_CL
Authordc.contributor.authorChen, Hsiao-Wen es_CL
Authordc.contributor.authorDickinson, Mark es_CL
Authordc.contributor.authorEisenhardt, Peter R. es_CL
Authordc.contributor.authorEspinoza, Juan es_CL
Authordc.contributor.authorGarnavich, Peter M. es_CL
Authordc.contributor.authorGonzález, David es_CL
Authordc.contributor.authorHarrison, Thomas E. es_CL
Authordc.contributor.authorHamuy Wackenhut, Mario es_CL
Authordc.contributor.authorVladimir, D. Ivanov es_CL
Authordc.contributor.authorKrzeminski, Wojtek es_CL
Authordc.contributor.authorKulesa, Craig es_CL
Authordc.contributor.authorMcCarthy, Patrick es_CL
Authordc.contributor.authorMoro Martín, Amaya es_CL
Authordc.contributor.authorMuena, César es_CL
Authordc.contributor.authorNoriega-Crespo, Alberto es_CL
Authordc.contributor.authorPersson, S. E. es_CL
Authordc.contributor.authorPinto, Philip A. es_CL
Authordc.contributor.authorRoth, Miguel es_CL
Authordc.contributor.authorRubenstein, Eric P. es_CL
Authordc.contributor.authorStanford, S. Adam es_CL
Authordc.contributor.authorStringfellow, Guy S. es_CL
Authordc.contributor.authorZapata, Abner es_CL
Authordc.contributor.authorPorter, Alain es_CL
Authordc.contributor.authorWischnjewsky, Marina 
Admission datedc.date.accessioned2014-01-10T18:39:18Z
Available datedc.date.available2014-01-10T18:39:18Z
Publication datedc.date.issued2004-12
Cita de ítemdc.identifier.citationThe Astronomical Journal, 128:3034–3052, 2004 Decemberen_US
Identifierdc.identifier.otherdoi: 10.1086/425629
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/126197
General notedc.descriptionArtículo de publicación ISI.en_US
Abstractdc.description.abstractWe present optical and/or infrared photometry of the Type Ia supernovae SN 1991T, SN 1991bg, SN 1999ek, SN 2001bt, SN 2001cn, SN 2001cz, and SN 2002bo. All but one of these supernovae have decline rate parameters, Deltam(15)(B), close to the median value of 1.1 for the whole class of Type Ia supernovae. The addition of these supernovae to the relationship between the near-infrared absolute magnitudes and Deltam(15)(B) strengthens the previous relationships we have found in that the maximum light absolute magnitudes are essentially independent of the decline rate parameter. (SN 1991bg, the prototype of the subclass of fast-declining Type Ia supernovae, is a special case.) The dispersion in the Hubble diagram in JHK is only similar to0.15 mag. The near-infrared properties of Type Ia supernovae continue to be excellent measures of the luminosity distances to the supernova host galaxies because of the need for only small corrections from the epoch of observation to maximum light, low dispersion in absolute magnitudes at maximum light, and the minimal reddening effects in the near-infrared.en_US
Lenguagedc.language.isoenen_US
Publisherdc.publisherIOP Publishingen_US
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Keywordsdc.subjectsupernovae: individual (SN 1991T, SN 1991bg, SN 1999ek, SN 2001bt, SN 2001cn, SN 2001cz, SN 2002bo)en_US
Títulodc.titleOptical and Infrared Photometry of the Type Ia Supernovae 1991T, 1991bg, 1999ek, 2001bt, 2001cn, 2001cz, and 2002boen_US
Document typedc.typeArtículo de revista


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Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile