SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle method

Autores
de Jaeger, T.; Galbany, L.; Filippenko, A. V.; González Gaitán, S.; Yasuda, N.; Maeda, K.; Tanaka, M.; Morokuma, T.; Moriya, T. J.; Tominaga, N.; Nomoto, Ken’ichi; Komiyama, Y.; Anderson, J. P.; Brink, T. G.; Carlberg, R. G.; Folatelli, Gaston; Hamuy, M.; Pignata, G.; Zheng, W.
Año de publicación
2017
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Although Type Ia supernova cosmology has now reached a mature state, it is important to develop as many independent methods as possible to understand the true nature of dark energy. Recent studies have shown that Type II supernovae (SNe II) offer such a path and could be used as alternative distance indicators. However, the majority of these studies were unable to extend the Hubble diagram above redshift z = 0.3 because of observational limitations. Here, we show that we are now ready to move beyond low redshifts and attempt high-redshift (z ≳ 0.3) SN II cosmology as a result of new-generation deep surveys such as the Subaru/Hyper Suprime-Cam survey. Applying the ´standard candle method´ to SN 2016jhj (z = 0.3398 ± 0.0002; discovered by HSC) together with a low-redshift sample, we are able to construct the highest-redshift SN II Hubble diagram to date with an observed dispersion of 0.27 mag (i.e. 12-13 per cent in distance). This work demonstrates the bright future of SN II cosmology in the coming era of large, wide-field surveys like that of the Large Synoptic Survey Telescope.
Fil: de Jaeger, T.. University of California at Berkeley; Estados Unidos
Fil: Galbany, L.. University of Pittsburgh at Johnstown; Estados Unidos
Fil: Filippenko, A. V.. University of California at Berkeley; Estados Unidos
Fil: González Gaitán, S.. Universidad de Chile; Chile
Fil: Yasuda, N.. University of Tokio; Japón
Fil: Maeda, K.. University of Tokio; Japón
Fil: Tanaka, M.. University of Tokio; Japón
Fil: Morokuma, T.. University of Tokio; Japón
Fil: Moriya, T. J.. National Astronomical Observatory of Japan; Japón
Fil: Tominaga, N.. University of Tokyo; Japón
Fil: Nomoto, Ken’ichi. University of Tokyo; Japón
Fil: Komiyama, Y.. National Astronomical Observatory of Japan; Japón
Fil: Anderson, J. P.. European Southern Observatory; Chile
Fil: Brink, T. G.. University of California at Berkeley; Estados Unidos
Fil: Carlberg, R. G.. University of Toronto; Canadá
Fil: Folatelli, Gaston. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. University of Tokyo; Japón
Fil: Hamuy, M.. Universidad de Chile; Chile
Fil: Pignata, G.. Universidad Andrés Bello; Chile
Fil: Zheng, W.. University of California at Berkeley; Estados Unidos
Materia
Supernova
Redshifts
Distance scale
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:11336/41203
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/41203
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle methodde Jaeger, T.Galbany, L.Filippenko, A. V.González Gaitán, S.Yasuda, N.Maeda, K.Tanaka, M.Morokuma, T.Moriya, T. J.Tominaga, N.Nomoto, Ken’ichiKomiyama, Y.Anderson, J. P.Brink, T. G.Carlberg, R. G.Folatelli, GastonHamuy, M.Pignata, G.Zheng, W.SupernovaRedshiftsDistance scalehttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Although Type Ia supernova cosmology has now reached a mature state, it is important to develop as many independent methods as possible to understand the true nature of dark energy. Recent studies have shown that Type II supernovae (SNe II) offer such a path and could be used as alternative distance indicators. However, the majority of these studies were unable to extend the Hubble diagram above redshift z = 0.3 because of observational limitations. Here, we show that we are now ready to move beyond low redshifts and attempt high-redshift (z ≳ 0.3) SN II cosmology as a result of new-generation deep surveys such as the Subaru/Hyper Suprime-Cam survey. Applying the ´standard candle method´ to SN 2016jhj (z = 0.3398 ± 0.0002; discovered by HSC) together with a low-redshift sample, we are able to construct the highest-redshift SN II Hubble diagram to date with an observed dispersion of 0.27 mag (i.e. 12-13 per cent in distance). This work demonstrates the bright future of SN II cosmology in the coming era of large, wide-field surveys like that of the Large Synoptic Survey Telescope.Fil: de Jaeger, T.. University of California at Berkeley; Estados UnidosFil: Galbany, L.. University of Pittsburgh at Johnstown; Estados UnidosFil: Filippenko, A. V.. University of California at Berkeley; Estados UnidosFil: González Gaitán, S.. Universidad de Chile; ChileFil: Yasuda, N.. University of Tokio; JapónFil: Maeda, K.. University of Tokio; JapónFil: Tanaka, M.. University of Tokio; JapónFil: Morokuma, T.. University of Tokio; JapónFil: Moriya, T. J.. National Astronomical Observatory of Japan; JapónFil: Tominaga, N.. University of Tokyo; JapónFil: Nomoto, Ken’ichi. University of Tokyo; JapónFil: Komiyama, Y.. National Astronomical Observatory of Japan; JapónFil: Anderson, J. P.. European Southern Observatory; ChileFil: Brink, T. G.. University of California at Berkeley; Estados UnidosFil: Carlberg, R. G.. University of Toronto; CanadáFil: Folatelli, Gaston. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. University of Tokyo; JapónFil: Hamuy, M.. Universidad de Chile; ChileFil: Pignata, G.. Universidad Andrés Bello; ChileFil: Zheng, W.. University of California at Berkeley; Estados UnidosWiley Blackwell Publishing, Inc2017-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/41203de Jaeger, T.; Galbany, L.; Filippenko, A. V.; González Gaitán, S.; Yasuda, N.; et al.; SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle method; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 472; 4; 12-2017; 4233-42430035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stx2300info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/472/4/4233/4107125info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:51:26Zoai:ri.conicet.gov.ar:11336/41203instacron: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 11:51:26.574CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle method
title SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle method
spellingShingle SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle method
de Jaeger, T.
Supernova
Redshifts
Distance scale
title_short SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle method
title_full SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle method
title_fullStr SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle method
title_full_unstemmed SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle method
title_sort SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle method
dc.creator.none.fl_str_mv de Jaeger, T.
Galbany, L.
Filippenko, A. V.
González Gaitán, S.
Yasuda, N.
Maeda, K.
Tanaka, M.
Morokuma, T.
Moriya, T. J.
Tominaga, N.
Nomoto, Ken’ichi
Komiyama, Y.
Anderson, J. P.
Brink, T. G.
Carlberg, R. G.
Folatelli, Gaston
Hamuy, M.
Pignata, G.
Zheng, W.
author de Jaeger, T.
author_facet de Jaeger, T.
Galbany, L.
Filippenko, A. V.
González Gaitán, S.
Yasuda, N.
Maeda, K.
Tanaka, M.
Morokuma, T.
Moriya, T. J.
Tominaga, N.
Nomoto, Ken’ichi
Komiyama, Y.
Anderson, J. P.
Brink, T. G.
Carlberg, R. G.
Folatelli, Gaston
Hamuy, M.
Pignata, G.
Zheng, W.
author_role author
author2 Galbany, L.
Filippenko, A. V.
González Gaitán, S.
Yasuda, N.
Maeda, K.
Tanaka, M.
Morokuma, T.
Moriya, T. J.
Tominaga, N.
Nomoto, Ken’ichi
Komiyama, Y.
Anderson, J. P.
Brink, T. G.
Carlberg, R. G.
Folatelli, Gaston
Hamuy, M.
Pignata, G.
Zheng, W.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Supernova
Redshifts
Distance scale
topic Supernova
Redshifts
Distance scale
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Although Type Ia supernova cosmology has now reached a mature state, it is important to develop as many independent methods as possible to understand the true nature of dark energy. Recent studies have shown that Type II supernovae (SNe II) offer such a path and could be used as alternative distance indicators. However, the majority of these studies were unable to extend the Hubble diagram above redshift z = 0.3 because of observational limitations. Here, we show that we are now ready to move beyond low redshifts and attempt high-redshift (z ≳ 0.3) SN II cosmology as a result of new-generation deep surveys such as the Subaru/Hyper Suprime-Cam survey. Applying the ´standard candle method´ to SN 2016jhj (z = 0.3398 ± 0.0002; discovered by HSC) together with a low-redshift sample, we are able to construct the highest-redshift SN II Hubble diagram to date with an observed dispersion of 0.27 mag (i.e. 12-13 per cent in distance). This work demonstrates the bright future of SN II cosmology in the coming era of large, wide-field surveys like that of the Large Synoptic Survey Telescope.
Fil: de Jaeger, T.. University of California at Berkeley; Estados Unidos
Fil: Galbany, L.. University of Pittsburgh at Johnstown; Estados Unidos
Fil: Filippenko, A. V.. University of California at Berkeley; Estados Unidos
Fil: González Gaitán, S.. Universidad de Chile; Chile
Fil: Yasuda, N.. University of Tokio; Japón
Fil: Maeda, K.. University of Tokio; Japón
Fil: Tanaka, M.. University of Tokio; Japón
Fil: Morokuma, T.. University of Tokio; Japón
Fil: Moriya, T. J.. National Astronomical Observatory of Japan; Japón
Fil: Tominaga, N.. University of Tokyo; Japón
Fil: Nomoto, Ken’ichi. University of Tokyo; Japón
Fil: Komiyama, Y.. National Astronomical Observatory of Japan; Japón
Fil: Anderson, J. P.. European Southern Observatory; Chile
Fil: Brink, T. G.. University of California at Berkeley; Estados Unidos
Fil: Carlberg, R. G.. University of Toronto; Canadá
Fil: Folatelli, Gaston. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. University of Tokyo; Japón
Fil: Hamuy, M.. Universidad de Chile; Chile
Fil: Pignata, G.. Universidad Andrés Bello; Chile
Fil: Zheng, W.. University of California at Berkeley; Estados Unidos
description Although Type Ia supernova cosmology has now reached a mature state, it is important to develop as many independent methods as possible to understand the true nature of dark energy. Recent studies have shown that Type II supernovae (SNe II) offer such a path and could be used as alternative distance indicators. However, the majority of these studies were unable to extend the Hubble diagram above redshift z = 0.3 because of observational limitations. Here, we show that we are now ready to move beyond low redshifts and attempt high-redshift (z ≳ 0.3) SN II cosmology as a result of new-generation deep surveys such as the Subaru/Hyper Suprime-Cam survey. Applying the ´standard candle method´ to SN 2016jhj (z = 0.3398 ± 0.0002; discovered by HSC) together with a low-redshift sample, we are able to construct the highest-redshift SN II Hubble diagram to date with an observed dispersion of 0.27 mag (i.e. 12-13 per cent in distance). This work demonstrates the bright future of SN II cosmology in the coming era of large, wide-field surveys like that of the Large Synoptic Survey Telescope.
publishDate 2017
dc.date.none.fl_str_mv 2017-12
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/11336/41203
de Jaeger, T.; Galbany, L.; Filippenko, A. V.; González Gaitán, S.; Yasuda, N.; et al.; SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle method; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 472; 4; 12-2017; 4233-4243
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/41203
identifier_str_mv de Jaeger, T.; Galbany, L.; Filippenko, A. V.; González Gaitán, S.; Yasuda, N.; et al.; SN 2016jhj at redshift 0.34: extending the Type II supernova Hubble diagram using the standard candle method; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 472; 4; 12-2017; 4233-4243
0035-8711
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stx2300
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article/472/4/4233/4107125
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 Wiley Blackwell Publishing, Inc
publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
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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