Defining photometric peculiar type Ia Supernovae

Autores
González Gaitán, S.; Hsiao, E. Y.; Pignata, G.; Förster, F.; Gutiérrez, C. P.; Bufano, F.; Galbany, L.; Folatelli, Gaston; Phillips, M. M.; Hamuy, M.; Anderson, J. P.; de Jaeger, T.
Año de publicación
2014
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present a new photometric identification technique for SN 1991bg-like type Ia supernovae (SNe Ia), i.e., objects with light curve characteristics such as later primary maxima and the absence of a secondary peak in redder filters. This method is capable of selecting this sub-group from the normal type Ia population. Furthermore, we find that recently identified peculiar sub-types such as SNe Iax and super-Chandrasekhar SNe Ia have photometric characteristics similar to 91bg-like SNe Ia, namely, the absence of secondary maxima and shoulders at longer wavelengths, and can also be classified with our technique. The similarity of these different SN Ia sub-groups perhaps suggests common physical conditions. This typing methodology permits the photometric identification of peculiar SNe Ia in large upcoming wide-field surveys either to study them further or to obtain a pure sample of normal SNe Ia for cosmological studies.
Fil: González Gaitán, S.. Instituto Milenio de Astrofísica; Chile. Universidad de Chile. Departamento de Astronomía; Chile
Fil: Hsiao, E. Y.. Carnegie Observatories; Chile
Fil: Pignata, G.. Instituto Milenio de Astrofísica; Chile. Universidad Andres Bello; Chile
Fil: Förster, F.. Instituto Milenio de Astrofísica; Chile. Universidad de Chile. Centro de Modelamiento Matemático; Chile
Fil: Gutiérrez, C. P.. Instituto Milenio de Astrofísica; Chile. Universidad de Chile. Departamento de Astronomía; Chile
Fil: Bufano, F.. Instituto Milenio de Astrofísica; Chile. Universidad Andres Bello; Chile
Fil: Galbany, L.. Instituto Milenio de Astrofísica; Chile. Universidad de Chile. Departamento de Astronomía; Chile
Fil: Folatelli, Gaston. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. University of Tokyo. Kavli Institute for the Physics and Mathematics of the Universe; Japón
Fil: Phillips, M. M.. Carnegie Observatories; Chile
Fil: Hamuy, M.. Instituto Milenio de Astrofísica; Chile. Universidad de Chile. Departamento de Astronomía; Chile
Fil: Anderson, J. P.. European Southern Observatory; Chile
Fil: de Jaeger, T.. Instituto Milenio de Astrofísica; Chile. Universidad de Chile. Departamento de Astronomía; Chile
Materia
Cosmology: Miscellaneous
Supernovae: General
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/10883
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/10883
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Defining photometric peculiar type Ia SupernovaeGonzález Gaitán, S.Hsiao, E. Y.Pignata, G.Förster, F.Gutiérrez, C. P.Bufano, F.Galbany, L.Folatelli, GastonPhillips, M. M.Hamuy, M.Anderson, J. P.de Jaeger, T.Cosmology: MiscellaneousSupernovae: Generalhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present a new photometric identification technique for SN 1991bg-like type Ia supernovae (SNe Ia), i.e., objects with light curve characteristics such as later primary maxima and the absence of a secondary peak in redder filters. This method is capable of selecting this sub-group from the normal type Ia population. Furthermore, we find that recently identified peculiar sub-types such as SNe Iax and super-Chandrasekhar SNe Ia have photometric characteristics similar to 91bg-like SNe Ia, namely, the absence of secondary maxima and shoulders at longer wavelengths, and can also be classified with our technique. The similarity of these different SN Ia sub-groups perhaps suggests common physical conditions. This typing methodology permits the photometric identification of peculiar SNe Ia in large upcoming wide-field surveys either to study them further or to obtain a pure sample of normal SNe Ia for cosmological studies.Fil: González Gaitán, S.. Instituto Milenio de Astrofísica; Chile. Universidad de Chile. Departamento de Astronomía; ChileFil: Hsiao, E. Y.. Carnegie Observatories; ChileFil: Pignata, G.. Instituto Milenio de Astrofísica; Chile. Universidad Andres Bello; ChileFil: Förster, F.. Instituto Milenio de Astrofísica; Chile. Universidad de Chile. Centro de Modelamiento Matemático; ChileFil: Gutiérrez, C. P.. Instituto Milenio de Astrofísica; Chile. Universidad de Chile. Departamento de Astronomía; ChileFil: Bufano, F.. Instituto Milenio de Astrofísica; Chile. Universidad Andres Bello; ChileFil: Galbany, L.. Instituto Milenio de Astrofísica; Chile. Universidad de Chile. Departamento de Astronomía; ChileFil: Folatelli, Gaston. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. University of Tokyo. Kavli Institute for the Physics and Mathematics of the Universe; JapónFil: Phillips, M. M.. Carnegie Observatories; ChileFil: Hamuy, M.. Instituto Milenio de Astrofísica; Chile. Universidad de Chile. Departamento de Astronomía; ChileFil: Anderson, J. P.. European Southern Observatory; ChileFil: de Jaeger, T.. Instituto Milenio de Astrofísica; Chile. Universidad de Chile. Departamento de Astronomía; ChileIop Publishing2014-11info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/10883González Gaitán, S.; Hsiao, E. Y.; Pignata, G.; Förster, F.; Gutiérrez, C. P.; et al.; Defining photometric peculiar type Ia Supernovae; Iop Publishing; Astrophysical Journal; 795; 2; 11-20140004-637X1538-4357enginfo:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/795/2/142info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/795/2/142/metainfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1409.4811info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:09:26Zoai:ri.conicet.gov.ar:11336/10883instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-22 11:09:27.265CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Defining photometric peculiar type Ia Supernovae
title Defining photometric peculiar type Ia Supernovae
spellingShingle Defining photometric peculiar type Ia Supernovae
González Gaitán, S.
Cosmology: Miscellaneous
Supernovae: General
title_short Defining photometric peculiar type Ia Supernovae
title_full Defining photometric peculiar type Ia Supernovae
title_fullStr Defining photometric peculiar type Ia Supernovae
title_full_unstemmed Defining photometric peculiar type Ia Supernovae
title_sort Defining photometric peculiar type Ia Supernovae
dc.creator.none.fl_str_mv González Gaitán, S.
Hsiao, E. Y.
Pignata, G.
Förster, F.
Gutiérrez, C. P.
Bufano, F.
Galbany, L.
Folatelli, Gaston
Phillips, M. M.
Hamuy, M.
Anderson, J. P.
de Jaeger, T.
author González Gaitán, S.
author_facet González Gaitán, S.
Hsiao, E. Y.
Pignata, G.
Förster, F.
Gutiérrez, C. P.
Bufano, F.
Galbany, L.
Folatelli, Gaston
Phillips, M. M.
Hamuy, M.
Anderson, J. P.
de Jaeger, T.
author_role author
author2 Hsiao, E. Y.
Pignata, G.
Förster, F.
Gutiérrez, C. P.
Bufano, F.
Galbany, L.
Folatelli, Gaston
Phillips, M. M.
Hamuy, M.
Anderson, J. P.
de Jaeger, T.
author2_role author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Cosmology: Miscellaneous
Supernovae: General
topic Cosmology: Miscellaneous
Supernovae: General
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We present a new photometric identification technique for SN 1991bg-like type Ia supernovae (SNe Ia), i.e., objects with light curve characteristics such as later primary maxima and the absence of a secondary peak in redder filters. This method is capable of selecting this sub-group from the normal type Ia population. Furthermore, we find that recently identified peculiar sub-types such as SNe Iax and super-Chandrasekhar SNe Ia have photometric characteristics similar to 91bg-like SNe Ia, namely, the absence of secondary maxima and shoulders at longer wavelengths, and can also be classified with our technique. The similarity of these different SN Ia sub-groups perhaps suggests common physical conditions. This typing methodology permits the photometric identification of peculiar SNe Ia in large upcoming wide-field surveys either to study them further or to obtain a pure sample of normal SNe Ia for cosmological studies.
Fil: González Gaitán, S.. Instituto Milenio de Astrofísica; Chile. Universidad de Chile. Departamento de Astronomía; Chile
Fil: Hsiao, E. Y.. Carnegie Observatories; Chile
Fil: Pignata, G.. Instituto Milenio de Astrofísica; Chile. Universidad Andres Bello; Chile
Fil: Förster, F.. Instituto Milenio de Astrofísica; Chile. Universidad de Chile. Centro de Modelamiento Matemático; Chile
Fil: Gutiérrez, C. P.. Instituto Milenio de Astrofísica; Chile. Universidad de Chile. Departamento de Astronomía; Chile
Fil: Bufano, F.. Instituto Milenio de Astrofísica; Chile. Universidad Andres Bello; Chile
Fil: Galbany, L.. Instituto Milenio de Astrofísica; Chile. Universidad de Chile. Departamento de Astronomía; Chile
Fil: Folatelli, Gaston. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. University of Tokyo. Kavli Institute for the Physics and Mathematics of the Universe; Japón
Fil: Phillips, M. M.. Carnegie Observatories; Chile
Fil: Hamuy, M.. Instituto Milenio de Astrofísica; Chile. Universidad de Chile. Departamento de Astronomía; Chile
Fil: Anderson, J. P.. European Southern Observatory; Chile
Fil: de Jaeger, T.. Instituto Milenio de Astrofísica; Chile. Universidad de Chile. Departamento de Astronomía; Chile
description We present a new photometric identification technique for SN 1991bg-like type Ia supernovae (SNe Ia), i.e., objects with light curve characteristics such as later primary maxima and the absence of a secondary peak in redder filters. This method is capable of selecting this sub-group from the normal type Ia population. Furthermore, we find that recently identified peculiar sub-types such as SNe Iax and super-Chandrasekhar SNe Ia have photometric characteristics similar to 91bg-like SNe Ia, namely, the absence of secondary maxima and shoulders at longer wavelengths, and can also be classified with our technique. The similarity of these different SN Ia sub-groups perhaps suggests common physical conditions. This typing methodology permits the photometric identification of peculiar SNe Ia in large upcoming wide-field surveys either to study them further or to obtain a pure sample of normal SNe Ia for cosmological studies.
publishDate 2014
dc.date.none.fl_str_mv 2014-11
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/10883
González Gaitán, S.; Hsiao, E. Y.; Pignata, G.; Förster, F.; Gutiérrez, C. P.; et al.; Defining photometric peculiar type Ia Supernovae; Iop Publishing; Astrophysical Journal; 795; 2; 11-2014
0004-637X
1538-4357
url http://hdl.handle.net/11336/10883
identifier_str_mv González Gaitán, S.; Hsiao, E. Y.; Pignata, G.; Förster, F.; Gutiérrez, C. P.; et al.; Defining photometric peculiar type Ia Supernovae; Iop Publishing; Astrophysical Journal; 795; 2; 11-2014
0004-637X
1538-4357
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/795/2/142
info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/795/2/142/meta
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1409.4811
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Iop Publishing
publisher.none.fl_str_mv Iop Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 12.982451

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