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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/10883
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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 Técnicas2025-09-29T09:40:49Zoai: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:34982025-09-29 09:40:49.54CONICET 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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1844613291449516032 |
score |
13.070432 |