A type II supernova Hubble Diagram from the CSP-I, SDSS-II, and SNLS surveys

Autores
Jaeger, T. De; González Gaitán, S.; Hamuy, M.; Galbany, L.; Anderson, J. P.; Phillips, M. M.; Stritzinger, M. D.; Carlberg, R. G.; Sullivan, M.; Gutiérrez, C. P.; Hook, I. M.; Howell, D. Andrew; Hsiao, E. Y.; Kuncarayakti, H.; Ruhlmann Kleider, V.; Folatelli, Gaston; Pritchet, C.; Basa, S.
Año de publicación
2017
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The coming era of large photometric wide-field surveys will increase the detection rate of supernovae by orders of magnitude. Such numbers will restrict spectroscopic follow-up in the vast majority of cases, and hence new methods based solely on photometric data must be developed. Here, we construct a complete Hubble diagram of Type II supernovae (SNe II) combining data from three different samples: the Carnegie Supernova Project-I, the Sloan Digital Sky Survey II SN, and the Supernova Legacy Survey. Applying the Photometric Color Method (PCM) to 73 SNe II with a redshift range of 0.01-0.5 and with no spectral information, we derive an intrinsic dispersion of 0.35 mag. A comparison with the Standard Candle Method (SCM) using 61 SNe II is also performed and an intrinsic dispersion in the Hubble diagram of 0.27 mag, i.e., 13% in distance uncertainties, is derived. Due to the lack of good statistics at higher redshifts for both methods, only weak constraints on the cosmological parameters are obtained. However, assuming a flat universe and using the PCM, we derive the universes matter density: m= 0.32 m+0.30 - 0.21 providing a new independent evidence for dark energy at the level of two sigma.
Fil: Jaeger, T. De. Millennium Institute Of Astrophysics; Chile. University of California at Berkeley; Estados Unidos. Universidad de Chile; Chile
Fil: González Gaitán, S.. Millennium Institute Of Astrophysics; Chile. Universidad de Chile; Chile
Fil: Hamuy, M.. Universidad de Chile; Chile. Millennium Institute Of Astrophysics; Chile
Fil: Galbany, L.. University of Pittsburgh at Johnstown; Estados Unidos. University of Pittsburgh; Estados Unidos
Fil: Anderson, J. P.. European Southern Observatory Santiago; Chile
Fil: Phillips, M. M.. Las Campanas Observatory; Chile
Fil: Stritzinger, M. D.. University Aarhus; Dinamarca
Fil: Carlberg, R. G.. University of Toronto; Canadá
Fil: Sullivan, M.. University of Southampton; Reino Unido
Fil: Gutiérrez, C. P.. European Southern Observatory Santiago; Chile. Millennium Institute Of Astrophysics; Chile. Universidad de Chile; Chile
Fil: Hook, I. M.. Lancaster University; Reino Unido
Fil: Howell, D. Andrew. Las Cumbres Observatory Global Telescope Network; Estados Unidos. University Of California, Santa Barbara; Estados Unidos
Fil: Hsiao, E. Y.. Las Campanas Observatory; Chile. University Aarhus; Dinamarca. Florida State University; Estados Unidos
Fil: Kuncarayakti, H.. Universidad de Chile; Chile. Millennium Institute Of Astrophysics; Chile
Fil: Ruhlmann Kleider, V.. Cea Saclay; Francia
Fil: Folatelli, Gaston. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Pritchet, C.. University Of Victoria; Canadá
Fil: Basa, S.. Laboratoire D'astrophysique de Marseille; Francia
Materia
Distances (galaxias)
Supernovae
Distance scale
Galaxies
Redshifts
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:11336/41103
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/41103
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling A type II supernova Hubble Diagram from the CSP-I, SDSS-II, and SNLS surveysJaeger, T. DeGonzález Gaitán, S.Hamuy, M.Galbany, L.Anderson, J. P.Phillips, M. M.Stritzinger, M. D.Carlberg, R. G.Sullivan, M.Gutiérrez, C. P.Hook, I. M.Howell, D. AndrewHsiao, E. Y.Kuncarayakti, H.Ruhlmann Kleider, V.Folatelli, GastonPritchet, C.Basa, S.Distances (galaxias)SupernovaeDistance scaleGalaxiesRedshiftshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The coming era of large photometric wide-field surveys will increase the detection rate of supernovae by orders of magnitude. Such numbers will restrict spectroscopic follow-up in the vast majority of cases, and hence new methods based solely on photometric data must be developed. Here, we construct a complete Hubble diagram of Type II supernovae (SNe II) combining data from three different samples: the Carnegie Supernova Project-I, the Sloan Digital Sky Survey II SN, and the Supernova Legacy Survey. Applying the Photometric Color Method (PCM) to 73 SNe II with a redshift range of 0.01-0.5 and with no spectral information, we derive an intrinsic dispersion of 0.35 mag. A comparison with the Standard Candle Method (SCM) using 61 SNe II is also performed and an intrinsic dispersion in the Hubble diagram of 0.27 mag, i.e., 13% in distance uncertainties, is derived. Due to the lack of good statistics at higher redshifts for both methods, only weak constraints on the cosmological parameters are obtained. However, assuming a flat universe and using the PCM, we derive the universes matter density: m= 0.32 m+0.30 - 0.21 providing a new independent evidence for dark energy at the level of two sigma.Fil: Jaeger, T. De. Millennium Institute Of Astrophysics; Chile. University of California at Berkeley; Estados Unidos. Universidad de Chile; ChileFil: González Gaitán, S.. Millennium Institute Of Astrophysics; Chile. Universidad de Chile; ChileFil: Hamuy, M.. Universidad de Chile; Chile. Millennium Institute Of Astrophysics; ChileFil: Galbany, L.. University of Pittsburgh at Johnstown; Estados Unidos. University of Pittsburgh; Estados UnidosFil: Anderson, J. P.. European Southern Observatory Santiago; ChileFil: Phillips, M. M.. Las Campanas Observatory; ChileFil: Stritzinger, M. D.. University Aarhus; DinamarcaFil: Carlberg, R. G.. University of Toronto; CanadáFil: Sullivan, M.. University of Southampton; Reino UnidoFil: Gutiérrez, C. P.. European Southern Observatory Santiago; Chile. Millennium Institute Of Astrophysics; Chile. Universidad de Chile; ChileFil: Hook, I. M.. Lancaster University; Reino UnidoFil: Howell, D. Andrew. Las Cumbres Observatory Global Telescope Network; Estados Unidos. University Of California, Santa Barbara; Estados UnidosFil: Hsiao, E. Y.. Las Campanas Observatory; Chile. University Aarhus; Dinamarca. Florida State University; Estados UnidosFil: Kuncarayakti, H.. Universidad de Chile; Chile. Millennium Institute Of Astrophysics; ChileFil: Ruhlmann Kleider, V.. Cea Saclay; FranciaFil: Folatelli, Gaston. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Pritchet, C.. University Of Victoria; CanadáFil: Basa, S.. Laboratoire D'astrophysique de Marseille; FranciaIOP Publishing2017-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/41103Jaeger, T. De; González Gaitán, S.; Hamuy, M.; Galbany, L.; Anderson, J. P.; et al.; A type II supernova Hubble Diagram from the CSP-I, SDSS-II, and SNLS surveys; IOP Publishing; Astrophysical Journal; 835; 2; 2-20170004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/835/2/166info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.3847/1538-4357/835/2/166/metainfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T09:59:19Zoai:ri.conicet.gov.ar:11336/41103instacron: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:34982025-09-03 09:59:19.908CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv A type II supernova Hubble Diagram from the CSP-I, SDSS-II, and SNLS surveys
title A type II supernova Hubble Diagram from the CSP-I, SDSS-II, and SNLS surveys
spellingShingle A type II supernova Hubble Diagram from the CSP-I, SDSS-II, and SNLS surveys
Jaeger, T. De
Distances (galaxias)
Supernovae
Distance scale
Galaxies
Redshifts
title_short A type II supernova Hubble Diagram from the CSP-I, SDSS-II, and SNLS surveys
title_full A type II supernova Hubble Diagram from the CSP-I, SDSS-II, and SNLS surveys
title_fullStr A type II supernova Hubble Diagram from the CSP-I, SDSS-II, and SNLS surveys
title_full_unstemmed A type II supernova Hubble Diagram from the CSP-I, SDSS-II, and SNLS surveys
title_sort A type II supernova Hubble Diagram from the CSP-I, SDSS-II, and SNLS surveys
dc.creator.none.fl_str_mv Jaeger, T. De
González Gaitán, S.
Hamuy, M.
Galbany, L.
Anderson, J. P.
Phillips, M. M.
Stritzinger, M. D.
Carlberg, R. G.
Sullivan, M.
Gutiérrez, C. P.
Hook, I. M.
Howell, D. Andrew
Hsiao, E. Y.
Kuncarayakti, H.
Ruhlmann Kleider, V.
Folatelli, Gaston
Pritchet, C.
Basa, S.
author Jaeger, T. De
author_facet Jaeger, T. De
González Gaitán, S.
Hamuy, M.
Galbany, L.
Anderson, J. P.
Phillips, M. M.
Stritzinger, M. D.
Carlberg, R. G.
Sullivan, M.
Gutiérrez, C. P.
Hook, I. M.
Howell, D. Andrew
Hsiao, E. Y.
Kuncarayakti, H.
Ruhlmann Kleider, V.
Folatelli, Gaston
Pritchet, C.
Basa, S.
author_role author
author2 González Gaitán, S.
Hamuy, M.
Galbany, L.
Anderson, J. P.
Phillips, M. M.
Stritzinger, M. D.
Carlberg, R. G.
Sullivan, M.
Gutiérrez, C. P.
Hook, I. M.
Howell, D. Andrew
Hsiao, E. Y.
Kuncarayakti, H.
Ruhlmann Kleider, V.
Folatelli, Gaston
Pritchet, C.
Basa, S.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Distances (galaxias)
Supernovae
Distance scale
Galaxies
Redshifts
topic Distances (galaxias)
Supernovae
Distance scale
Galaxies
Redshifts
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The coming era of large photometric wide-field surveys will increase the detection rate of supernovae by orders of magnitude. Such numbers will restrict spectroscopic follow-up in the vast majority of cases, and hence new methods based solely on photometric data must be developed. Here, we construct a complete Hubble diagram of Type II supernovae (SNe II) combining data from three different samples: the Carnegie Supernova Project-I, the Sloan Digital Sky Survey II SN, and the Supernova Legacy Survey. Applying the Photometric Color Method (PCM) to 73 SNe II with a redshift range of 0.01-0.5 and with no spectral information, we derive an intrinsic dispersion of 0.35 mag. A comparison with the Standard Candle Method (SCM) using 61 SNe II is also performed and an intrinsic dispersion in the Hubble diagram of 0.27 mag, i.e., 13% in distance uncertainties, is derived. Due to the lack of good statistics at higher redshifts for both methods, only weak constraints on the cosmological parameters are obtained. However, assuming a flat universe and using the PCM, we derive the universes matter density: m= 0.32 m+0.30 - 0.21 providing a new independent evidence for dark energy at the level of two sigma.
Fil: Jaeger, T. De. Millennium Institute Of Astrophysics; Chile. University of California at Berkeley; Estados Unidos. Universidad de Chile; Chile
Fil: González Gaitán, S.. Millennium Institute Of Astrophysics; Chile. Universidad de Chile; Chile
Fil: Hamuy, M.. Universidad de Chile; Chile. Millennium Institute Of Astrophysics; Chile
Fil: Galbany, L.. University of Pittsburgh at Johnstown; Estados Unidos. University of Pittsburgh; Estados Unidos
Fil: Anderson, J. P.. European Southern Observatory Santiago; Chile
Fil: Phillips, M. M.. Las Campanas Observatory; Chile
Fil: Stritzinger, M. D.. University Aarhus; Dinamarca
Fil: Carlberg, R. G.. University of Toronto; Canadá
Fil: Sullivan, M.. University of Southampton; Reino Unido
Fil: Gutiérrez, C. P.. European Southern Observatory Santiago; Chile. Millennium Institute Of Astrophysics; Chile. Universidad de Chile; Chile
Fil: Hook, I. M.. Lancaster University; Reino Unido
Fil: Howell, D. Andrew. Las Cumbres Observatory Global Telescope Network; Estados Unidos. University Of California, Santa Barbara; Estados Unidos
Fil: Hsiao, E. Y.. Las Campanas Observatory; Chile. University Aarhus; Dinamarca. Florida State University; Estados Unidos
Fil: Kuncarayakti, H.. Universidad de Chile; Chile. Millennium Institute Of Astrophysics; Chile
Fil: Ruhlmann Kleider, V.. Cea Saclay; Francia
Fil: Folatelli, Gaston. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Pritchet, C.. University Of Victoria; Canadá
Fil: Basa, S.. Laboratoire D'astrophysique de Marseille; Francia
description The coming era of large photometric wide-field surveys will increase the detection rate of supernovae by orders of magnitude. Such numbers will restrict spectroscopic follow-up in the vast majority of cases, and hence new methods based solely on photometric data must be developed. Here, we construct a complete Hubble diagram of Type II supernovae (SNe II) combining data from three different samples: the Carnegie Supernova Project-I, the Sloan Digital Sky Survey II SN, and the Supernova Legacy Survey. Applying the Photometric Color Method (PCM) to 73 SNe II with a redshift range of 0.01-0.5 and with no spectral information, we derive an intrinsic dispersion of 0.35 mag. A comparison with the Standard Candle Method (SCM) using 61 SNe II is also performed and an intrinsic dispersion in the Hubble diagram of 0.27 mag, i.e., 13% in distance uncertainties, is derived. Due to the lack of good statistics at higher redshifts for both methods, only weak constraints on the cosmological parameters are obtained. However, assuming a flat universe and using the PCM, we derive the universes matter density: m= 0.32 m+0.30 - 0.21 providing a new independent evidence for dark energy at the level of two sigma.
publishDate 2017
dc.date.none.fl_str_mv 2017-02
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/11336/41103
Jaeger, T. De; González Gaitán, S.; Hamuy, M.; Galbany, L.; Anderson, J. P.; et al.; A type II supernova Hubble Diagram from the CSP-I, SDSS-II, and SNLS surveys; IOP Publishing; Astrophysical Journal; 835; 2; 2-2017
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/41103
identifier_str_mv Jaeger, T. De; González Gaitán, S.; Hamuy, M.; Galbany, L.; Anderson, J. P.; et al.; A type II supernova Hubble Diagram from the CSP-I, SDSS-II, and SNLS surveys; IOP Publishing; Astrophysical Journal; 835; 2; 2-2017
0004-637X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/835/2/166
info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.3847/1538-4357/835/2/166/meta
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 13.13397

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