A Hubble diagram from type II supernovae based solely on photometry: the photometric color method

Autores
De Jaeger, T.; González Gaitán, S.; Anderson, J. P.; Galbany, L.; Hamuy, M.; Phillips, M. M.; Stritzinger, M. D.; Gutiérrez, C. P.; Bolt, L.; Burns, C. R.; Campillay, A.; Castellón, S.; Contreras, C.; Folatelli, Gaston; Freedman, W. L.; Hsiao, E. Y.; Krisciunas, K.; Krzeminski, W.; Kuncarayakti, H.; Morrell, N.; Olivares E. F.; Persson, S. E.; Suntzeff, N.
Año de publicación
2015
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present a Hubble diagram of SNe II using corrected magnitudes derived only from photometry, with no input of spectral information. We use a data set from the Carnegie Supernovae Project I for which optical and near-infrared light curves were obtained. The apparent magnitude is corrected by two observables, one corresponding to the slope of the plateau in the V band and the second a color term. We obtain a dispersion of 0.44 mag using a combination of the (V - i) color and the r band and we are able to reduce the dispersion to 0.39 mag using our golden sample. A comparison of our photometric color method (PCM) with the standardized candle method (SCM) is also performed. The dispersion obtained for the SCM (which uses both photometric and spectroscopic information) is 0.29 mag, which compares with 0.43 mag from the PCM for the same SN sample. The construction of a photometric Hubble diagram is of high importance in the coming era of large photometric wide-field surveys, which will increase the detection rate of supernovae by orders of magnitude. Such numbers will prohibit spectroscopic follow up in the vast majority of cases, and hence methods must be deployed which can proceed using solely photometric data.
Fil: De Jaeger, T. . Universidad de Chile; Chile
Fil: González Gaitán, S.. Universidad de Chile; Chile
Fil: Anderson, J. P. . European Southern Observatory; Chile
Fil: Galbany, L.. Universidad de Chile; Chile
Fil: Hamuy, M.. Universidad de Chile; Chile
Fil: Phillips, M. M. . Carnegie Observatories. Las Campanas Observatory; Chile
Fil: Stritzinger, M. D.. Aarhus University; Dinamarca
Fil: Gutiérrez, C. P.. Universidad de Chile; Chile
Fil: Bolt, L.. Universität Bonn; Alemania
Fil: Burns, C. R. . Observatories of the Carnegie Institution for Science; Estados Unidos
Fil: Campillay, A.. Carnegie Observatories. Las Campanas Observatory; Chile
Fil: Castellón, S.. Carnegie Observatories. Las Campanas Observatory; Chile
Fil: Contreras, C.. Aarhus University; Dinamarca
Fil: Folatelli, Gaston. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina. University of Tokyo; Japón
Fil: Freedman, W. L. . University Of Chicago; Estados Unidos
Fil: Hsiao, E. Y. . Carnegie Observatories. Las Campanas Observatory; Chile
Fil: Krisciunas, K.. Texas AyM University; Estados Unidos
Fil: Krzeminski, W.. N. Copernicus Astronomical Center; Polonia
Fil: Kuncarayakti, H.. Universidad de Chile; Chile
Fil: Morrell, N.. Carnegie Observatories. Las Campanas Observatory; Chile
Fil: Olivares E. F.. Universidad de Chile; Chile
Fil: Persson, S. E. . Observatories of the Carnegie Institution for Science; Estados Unidos
Fil: Suntzeff, N.. Texas AyM University; Estados Unidos
Materia
Distance Scale
Galaxis
Distances
Supernovae
Redshift
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:11336/13772
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/13772
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling A Hubble diagram from type II supernovae based solely on photometry: the photometric color methodDe Jaeger, T. González Gaitán, S.Anderson, J. P. Galbany, L.Hamuy, M.Phillips, M. M. Stritzinger, M. D.Gutiérrez, C. P.Bolt, L.Burns, C. R. Campillay, A.Castellón, S.Contreras, C.Folatelli, GastonFreedman, W. L. Hsiao, E. Y. Krisciunas, K.Krzeminski, W.Kuncarayakti, H.Morrell, N.Olivares E. F.Persson, S. E. Suntzeff, N.Distance ScaleGalaxisDistancesSupernovaeRedshifthttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present a Hubble diagram of SNe II using corrected magnitudes derived only from photometry, with no input of spectral information. We use a data set from the Carnegie Supernovae Project I for which optical and near-infrared light curves were obtained. The apparent magnitude is corrected by two observables, one corresponding to the slope of the plateau in the V band and the second a color term. We obtain a dispersion of 0.44 mag using a combination of the (V - i) color and the r band and we are able to reduce the dispersion to 0.39 mag using our golden sample. A comparison of our photometric color method (PCM) with the standardized candle method (SCM) is also performed. The dispersion obtained for the SCM (which uses both photometric and spectroscopic information) is 0.29 mag, which compares with 0.43 mag from the PCM for the same SN sample. The construction of a photometric Hubble diagram is of high importance in the coming era of large photometric wide-field surveys, which will increase the detection rate of supernovae by orders of magnitude. Such numbers will prohibit spectroscopic follow up in the vast majority of cases, and hence methods must be deployed which can proceed using solely photometric data.Fil: De Jaeger, T. . Universidad de Chile; ChileFil: González Gaitán, S.. Universidad de Chile; ChileFil: Anderson, J. P. . European Southern Observatory; ChileFil: Galbany, L.. Universidad de Chile; ChileFil: Hamuy, M.. Universidad de Chile; ChileFil: Phillips, M. M. . Carnegie Observatories. Las Campanas Observatory; ChileFil: Stritzinger, M. D.. Aarhus University; DinamarcaFil: Gutiérrez, C. P.. Universidad de Chile; ChileFil: Bolt, L.. Universität Bonn; AlemaniaFil: Burns, C. R. . Observatories of the Carnegie Institution for Science; Estados UnidosFil: Campillay, A.. Carnegie Observatories. Las Campanas Observatory; ChileFil: Castellón, S.. Carnegie Observatories. Las Campanas Observatory; ChileFil: Contreras, C.. Aarhus University; DinamarcaFil: Folatelli, Gaston. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina. University of Tokyo; JapónFil: Freedman, W. L. . University Of Chicago; Estados UnidosFil: Hsiao, E. Y. . Carnegie Observatories. Las Campanas Observatory; ChileFil: Krisciunas, K.. Texas AyM University; Estados UnidosFil: Krzeminski, W.. N. Copernicus Astronomical Center; PoloniaFil: Kuncarayakti, H.. Universidad de Chile; ChileFil: Morrell, N.. Carnegie Observatories. Las Campanas Observatory; ChileFil: Olivares E. F.. Universidad de Chile; ChileFil: Persson, S. E. . Observatories of the Carnegie Institution for Science; Estados UnidosFil: Suntzeff, N.. Texas AyM University; Estados UnidosIop Publishing2015-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/13772De Jaeger, T. ; González Gaitán, S.; Anderson, J. P. ; Galbany, L.; Hamuy, M.; et al.; A Hubble diagram from type II supernovae based solely on photometry: the photometric color method; Iop Publishing; Astrophysical Journal; 815; 2; 12-2015; 121-1430004-637Xenginfo:eu-repo/semantics/altIdentifier/url/https://doi.org/10.1088/0004-637X/815/2/121info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/815/2/121info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:39:58Zoai:ri.conicet.gov.ar:11336/13772instacron: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 11:39:58.594CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv A Hubble diagram from type II supernovae based solely on photometry: the photometric color method
title A Hubble diagram from type II supernovae based solely on photometry: the photometric color method
spellingShingle A Hubble diagram from type II supernovae based solely on photometry: the photometric color method
De Jaeger, T.
Distance Scale
Galaxis
Distances
Supernovae
Redshift
title_short A Hubble diagram from type II supernovae based solely on photometry: the photometric color method
title_full A Hubble diagram from type II supernovae based solely on photometry: the photometric color method
title_fullStr A Hubble diagram from type II supernovae based solely on photometry: the photometric color method
title_full_unstemmed A Hubble diagram from type II supernovae based solely on photometry: the photometric color method
title_sort A Hubble diagram from type II supernovae based solely on photometry: the photometric color method
dc.creator.none.fl_str_mv De Jaeger, T.
González Gaitán, S.
Anderson, J. P.
Galbany, L.
Hamuy, M.
Phillips, M. M.
Stritzinger, M. D.
Gutiérrez, C. P.
Bolt, L.
Burns, C. R.
Campillay, A.
Castellón, S.
Contreras, C.
Folatelli, Gaston
Freedman, W. L.
Hsiao, E. Y.
Krisciunas, K.
Krzeminski, W.
Kuncarayakti, H.
Morrell, N.
Olivares E. F.
Persson, S. E.
Suntzeff, N.
author De Jaeger, T.
author_facet De Jaeger, T.
González Gaitán, S.
Anderson, J. P.
Galbany, L.
Hamuy, M.
Phillips, M. M.
Stritzinger, M. D.
Gutiérrez, C. P.
Bolt, L.
Burns, C. R.
Campillay, A.
Castellón, S.
Contreras, C.
Folatelli, Gaston
Freedman, W. L.
Hsiao, E. Y.
Krisciunas, K.
Krzeminski, W.
Kuncarayakti, H.
Morrell, N.
Olivares E. F.
Persson, S. E.
Suntzeff, N.
author_role author
author2 González Gaitán, S.
Anderson, J. P.
Galbany, L.
Hamuy, M.
Phillips, M. M.
Stritzinger, M. D.
Gutiérrez, C. P.
Bolt, L.
Burns, C. R.
Campillay, A.
Castellón, S.
Contreras, C.
Folatelli, Gaston
Freedman, W. L.
Hsiao, E. Y.
Krisciunas, K.
Krzeminski, W.
Kuncarayakti, H.
Morrell, N.
Olivares E. F.
Persson, S. E.
Suntzeff, N.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Distance Scale
Galaxis
Distances
Supernovae
Redshift
topic Distance Scale
Galaxis
Distances
Supernovae
Redshift
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 Hubble diagram of SNe II using corrected magnitudes derived only from photometry, with no input of spectral information. We use a data set from the Carnegie Supernovae Project I for which optical and near-infrared light curves were obtained. The apparent magnitude is corrected by two observables, one corresponding to the slope of the plateau in the V band and the second a color term. We obtain a dispersion of 0.44 mag using a combination of the (V - i) color and the r band and we are able to reduce the dispersion to 0.39 mag using our golden sample. A comparison of our photometric color method (PCM) with the standardized candle method (SCM) is also performed. The dispersion obtained for the SCM (which uses both photometric and spectroscopic information) is 0.29 mag, which compares with 0.43 mag from the PCM for the same SN sample. The construction of a photometric Hubble diagram is of high importance in the coming era of large photometric wide-field surveys, which will increase the detection rate of supernovae by orders of magnitude. Such numbers will prohibit spectroscopic follow up in the vast majority of cases, and hence methods must be deployed which can proceed using solely photometric data.
Fil: De Jaeger, T. . Universidad de Chile; Chile
Fil: González Gaitán, S.. Universidad de Chile; Chile
Fil: Anderson, J. P. . European Southern Observatory; Chile
Fil: Galbany, L.. Universidad de Chile; Chile
Fil: Hamuy, M.. Universidad de Chile; Chile
Fil: Phillips, M. M. . Carnegie Observatories. Las Campanas Observatory; Chile
Fil: Stritzinger, M. D.. Aarhus University; Dinamarca
Fil: Gutiérrez, C. P.. Universidad de Chile; Chile
Fil: Bolt, L.. Universität Bonn; Alemania
Fil: Burns, C. R. . Observatories of the Carnegie Institution for Science; Estados Unidos
Fil: Campillay, A.. Carnegie Observatories. Las Campanas Observatory; Chile
Fil: Castellón, S.. Carnegie Observatories. Las Campanas Observatory; Chile
Fil: Contreras, C.. Aarhus University; Dinamarca
Fil: Folatelli, Gaston. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto de Astrofísica de La Plata; Argentina. University of Tokyo; Japón
Fil: Freedman, W. L. . University Of Chicago; Estados Unidos
Fil: Hsiao, E. Y. . Carnegie Observatories. Las Campanas Observatory; Chile
Fil: Krisciunas, K.. Texas AyM University; Estados Unidos
Fil: Krzeminski, W.. N. Copernicus Astronomical Center; Polonia
Fil: Kuncarayakti, H.. Universidad de Chile; Chile
Fil: Morrell, N.. Carnegie Observatories. Las Campanas Observatory; Chile
Fil: Olivares E. F.. Universidad de Chile; Chile
Fil: Persson, S. E. . Observatories of the Carnegie Institution for Science; Estados Unidos
Fil: Suntzeff, N.. Texas AyM University; Estados Unidos
description We present a Hubble diagram of SNe II using corrected magnitudes derived only from photometry, with no input of spectral information. We use a data set from the Carnegie Supernovae Project I for which optical and near-infrared light curves were obtained. The apparent magnitude is corrected by two observables, one corresponding to the slope of the plateau in the V band and the second a color term. We obtain a dispersion of 0.44 mag using a combination of the (V - i) color and the r band and we are able to reduce the dispersion to 0.39 mag using our golden sample. A comparison of our photometric color method (PCM) with the standardized candle method (SCM) is also performed. The dispersion obtained for the SCM (which uses both photometric and spectroscopic information) is 0.29 mag, which compares with 0.43 mag from the PCM for the same SN sample. The construction of a photometric Hubble diagram is of high importance in the coming era of large photometric wide-field surveys, which will increase the detection rate of supernovae by orders of magnitude. Such numbers will prohibit spectroscopic follow up in the vast majority of cases, and hence methods must be deployed which can proceed using solely photometric data.
publishDate 2015
dc.date.none.fl_str_mv 2015-12
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/11336/13772
De Jaeger, T. ; González Gaitán, S.; Anderson, J. P. ; Galbany, L.; Hamuy, M.; et al.; A Hubble diagram from type II supernovae based solely on photometry: the photometric color method; Iop Publishing; Astrophysical Journal; 815; 2; 12-2015; 121-143
0004-637X
url http://hdl.handle.net/11336/13772
identifier_str_mv De Jaeger, T. ; González Gaitán, S.; Anderson, J. P. ; Galbany, L.; Hamuy, M.; et al.; A Hubble diagram from type II supernovae based solely on photometry: the photometric color method; Iop Publishing; Astrophysical Journal; 815; 2; 12-2015; 121-143
0004-637X
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://doi.org/10.1088/0004-637X/815/2/121
info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/815/2/121
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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