Carnegie Supernova Project-II: Near-infrared Spectroscopy of Stripped-envelope Core-collapse Supernovae

Autores
Shahbandeh, M.; Hsiao, E. Y.; Ashall, C.; Teffs, J.; Hoeflich, P.; Morrell, N.; Phillips, M. M.; Anderson, J. P.; Baron, E.; Burns, C. R.; Contreras, C.; Davis, S.; Diamond, T. R.; Folatelli, Gaston; Galbany, L.; Gall, C.; Hachinger, S.; Holmbo, S.; Karamehmetoglu, E.; Kasliwal, M. M.; Kirshner, R. P.; Krisciunas, K.; Kumar, S.; Lu, J.; Marion, G. H.; Mazzali, P. A.; Piro, A. L.; Sand, D. J.; Stritzinger, M. D.; Suntzeff, N. B.; Taddia, F.; Uddin, S. A.
Año de publicación
2022
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present 75 near-infrared (NIR; 0.8-2.5 μm) spectra of 34 stripped-envelope core-collapse supernovae (SESNe) obtained by the Carnegie Supernova Project-II (CSP-II), encompassing optical spectroscopic Types IIb, Ib, Ic, and Ic-BL. The spectra range in phase from pre-maximum to 80 days past maximum. This unique data set constitutes the largest NIR spectroscopic sample of SESNe to date. NIR spectroscopy provides observables with additional information that is not available in the optical. Specifically, the NIR contains the strong lines of He i and allows a more detailed look at whether Type Ic supernovae are completely stripped of their outer He layer. The NIR spectra of SESNe have broad similarities, but closer examination through statistical means reveals a strong dichotomy between NIR "He-rich"and "He-poor"SNe. These NIR subgroups correspond almost perfectly to the optical IIb/Ib and Ic/Ic-BL types, respectively. The largest difference between the two groups is observed in the 2 μm region, near the He i λ2.0581 μm line. The division between the two groups is not an arbitrary one along a continuous sequence. Early spectra of He-rich SESNe show much stronger He i λ2.0581 μm absorption compared to the He-poor group, but with a wide range of profile shapes. The same line also provides evidence for trace amounts of He in half of our SNe in the He-poor group.
Fil: Shahbandeh, M.. Florida State University; Estados Unidos
Fil: Hsiao, E. Y.. Florida State University; Estados Unidos
Fil: Ashall, C.. University Hawaii Institute For Astronomy; Estados Unidos
Fil: Teffs, J.. Liverpool John Moores University; Reino Unido
Fil: Hoeflich, P.. Florida State University; Estados Unidos
Fil: Morrell, N.. Las Campanas Observatory; Chile
Fil: Phillips, M. M.. Las Campanas Observatory; Chile
Fil: Anderson, J. P.. European Southern Observatory Santiago; Chile
Fil: Baron, E.. No especifíca;
Fil: Burns, C. R.. No especifíca;
Fil: Contreras, C.. Las Campanas Observatory; Chile
Fil: Davis, S.. University of California at Davis; Estados Unidos
Fil: Diamond, T. R.. Private Astronomer; Estados Unidos
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: Galbany, L.. Consejo Superior de Investigaciones Científicas; España
Fil: Gall, C.. No especifíca;
Fil: Hachinger, S.. No especifíca;
Fil: Holmbo, S.. University Aarhus; Dinamarca
Fil: Karamehmetoglu, E.. University Aarhus; Dinamarca
Fil: Kasliwal, M. M.. California Institute of Technology; Estados Unidos
Fil: Kirshner, R. P.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Krisciunas, K.. Texas A&M University; Estados Unidos
Fil: Kumar, S.. Florida State University; Estados Unidos
Fil: Lu, J.. Florida State University; Estados Unidos
Fil: Marion, G. H.. University of Texas at Austin; Estados Unidos
Fil: Mazzali, P. A.. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; Alemania
Fil: Piro, A. L.. No especifíca;
Fil: Sand, D. J.. University of Arizona; Estados Unidos
Fil: Stritzinger, M. D.. University Aarhus; Dinamarca
Fil: Suntzeff, N. B.. Texas A&M University; Estados Unidos
Fil: Taddia, F.. University Aarhus; Dinamarca
Fil: Uddin, S. A.. Texas A&M University; Estados Unidos
Materia
SUPERNOVAE
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:11336/210879

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network_name_str CONICET Digital (CONICET)
spelling Carnegie Supernova Project-II: Near-infrared Spectroscopy of Stripped-envelope Core-collapse SupernovaeShahbandeh, M.Hsiao, E. Y.Ashall, C.Teffs, J.Hoeflich, P.Morrell, N.Phillips, M. M.Anderson, J. P.Baron, E.Burns, C. R.Contreras, C.Davis, S.Diamond, T. R.Folatelli, GastonGalbany, L.Gall, C.Hachinger, S.Holmbo, S.Karamehmetoglu, E.Kasliwal, M. M.Kirshner, R. P.Krisciunas, K.Kumar, S.Lu, J.Marion, G. H.Mazzali, P. A.Piro, A. L.Sand, D. J.Stritzinger, M. D.Suntzeff, N. B.Taddia, F.Uddin, S. A.SUPERNOVAEhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present 75 near-infrared (NIR; 0.8-2.5 μm) spectra of 34 stripped-envelope core-collapse supernovae (SESNe) obtained by the Carnegie Supernova Project-II (CSP-II), encompassing optical spectroscopic Types IIb, Ib, Ic, and Ic-BL. The spectra range in phase from pre-maximum to 80 days past maximum. This unique data set constitutes the largest NIR spectroscopic sample of SESNe to date. NIR spectroscopy provides observables with additional information that is not available in the optical. Specifically, the NIR contains the strong lines of He i and allows a more detailed look at whether Type Ic supernovae are completely stripped of their outer He layer. The NIR spectra of SESNe have broad similarities, but closer examination through statistical means reveals a strong dichotomy between NIR "He-rich"and "He-poor"SNe. These NIR subgroups correspond almost perfectly to the optical IIb/Ib and Ic/Ic-BL types, respectively. The largest difference between the two groups is observed in the 2 μm region, near the He i λ2.0581 μm line. The division between the two groups is not an arbitrary one along a continuous sequence. Early spectra of He-rich SESNe show much stronger He i λ2.0581 μm absorption compared to the He-poor group, but with a wide range of profile shapes. The same line also provides evidence for trace amounts of He in half of our SNe in the He-poor group.Fil: Shahbandeh, M.. Florida State University; Estados UnidosFil: Hsiao, E. Y.. Florida State University; Estados UnidosFil: Ashall, C.. University Hawaii Institute For Astronomy; Estados UnidosFil: Teffs, J.. Liverpool John Moores University; Reino UnidoFil: Hoeflich, P.. Florida State University; Estados UnidosFil: Morrell, N.. Las Campanas Observatory; ChileFil: Phillips, M. M.. Las Campanas Observatory; ChileFil: Anderson, J. P.. European Southern Observatory Santiago; ChileFil: Baron, E.. No especifíca;Fil: Burns, C. R.. No especifíca;Fil: Contreras, C.. Las Campanas Observatory; ChileFil: Davis, S.. University of California at Davis; Estados UnidosFil: Diamond, T. R.. Private Astronomer; Estados UnidosFil: 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: Galbany, L.. Consejo Superior de Investigaciones Científicas; EspañaFil: Gall, C.. No especifíca;Fil: Hachinger, S.. No especifíca;Fil: Holmbo, S.. University Aarhus; DinamarcaFil: Karamehmetoglu, E.. University Aarhus; DinamarcaFil: Kasliwal, M. M.. California Institute of Technology; Estados UnidosFil: Kirshner, R. P.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Krisciunas, K.. Texas A&M University; Estados UnidosFil: Kumar, S.. Florida State University; Estados UnidosFil: Lu, J.. Florida State University; Estados UnidosFil: Marion, G. H.. University of Texas at Austin; Estados UnidosFil: Mazzali, P. A.. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; AlemaniaFil: Piro, A. L.. No especifíca;Fil: Sand, D. J.. University of Arizona; Estados UnidosFil: Stritzinger, M. D.. University Aarhus; DinamarcaFil: Suntzeff, N. B.. Texas A&M University; Estados UnidosFil: Taddia, F.. University Aarhus; DinamarcaFil: Uddin, S. A.. Texas A&M University; Estados UnidosIOP Publishing2022-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/210879Shahbandeh, M.; Hsiao, E. Y.; Ashall, C.; Teffs, J.; Hoeflich, P.; et al.; Carnegie Supernova Project-II: Near-infrared Spectroscopy of Stripped-envelope Core-collapse Supernovae; IOP Publishing; Astrophysical Journal; 925; 2; 2-2022; 1-240004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ac4030info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:39:34Zoai:ri.conicet.gov.ar:11336/210879instacron: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 09:39:34.463CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Carnegie Supernova Project-II: Near-infrared Spectroscopy of Stripped-envelope Core-collapse Supernovae
title Carnegie Supernova Project-II: Near-infrared Spectroscopy of Stripped-envelope Core-collapse Supernovae
spellingShingle Carnegie Supernova Project-II: Near-infrared Spectroscopy of Stripped-envelope Core-collapse Supernovae
Shahbandeh, M.
SUPERNOVAE
title_short Carnegie Supernova Project-II: Near-infrared Spectroscopy of Stripped-envelope Core-collapse Supernovae
title_full Carnegie Supernova Project-II: Near-infrared Spectroscopy of Stripped-envelope Core-collapse Supernovae
title_fullStr Carnegie Supernova Project-II: Near-infrared Spectroscopy of Stripped-envelope Core-collapse Supernovae
title_full_unstemmed Carnegie Supernova Project-II: Near-infrared Spectroscopy of Stripped-envelope Core-collapse Supernovae
title_sort Carnegie Supernova Project-II: Near-infrared Spectroscopy of Stripped-envelope Core-collapse Supernovae
dc.creator.none.fl_str_mv Shahbandeh, M.
Hsiao, E. Y.
Ashall, C.
Teffs, J.
Hoeflich, P.
Morrell, N.
Phillips, M. M.
Anderson, J. P.
Baron, E.
Burns, C. R.
Contreras, C.
Davis, S.
Diamond, T. R.
Folatelli, Gaston
Galbany, L.
Gall, C.
Hachinger, S.
Holmbo, S.
Karamehmetoglu, E.
Kasliwal, M. M.
Kirshner, R. P.
Krisciunas, K.
Kumar, S.
Lu, J.
Marion, G. H.
Mazzali, P. A.
Piro, A. L.
Sand, D. J.
Stritzinger, M. D.
Suntzeff, N. B.
Taddia, F.
Uddin, S. A.
author Shahbandeh, M.
author_facet Shahbandeh, M.
Hsiao, E. Y.
Ashall, C.
Teffs, J.
Hoeflich, P.
Morrell, N.
Phillips, M. M.
Anderson, J. P.
Baron, E.
Burns, C. R.
Contreras, C.
Davis, S.
Diamond, T. R.
Folatelli, Gaston
Galbany, L.
Gall, C.
Hachinger, S.
Holmbo, S.
Karamehmetoglu, E.
Kasliwal, M. M.
Kirshner, R. P.
Krisciunas, K.
Kumar, S.
Lu, J.
Marion, G. H.
Mazzali, P. A.
Piro, A. L.
Sand, D. J.
Stritzinger, M. D.
Suntzeff, N. B.
Taddia, F.
Uddin, S. A.
author_role author
author2 Hsiao, E. Y.
Ashall, C.
Teffs, J.
Hoeflich, P.
Morrell, N.
Phillips, M. M.
Anderson, J. P.
Baron, E.
Burns, C. R.
Contreras, C.
Davis, S.
Diamond, T. R.
Folatelli, Gaston
Galbany, L.
Gall, C.
Hachinger, S.
Holmbo, S.
Karamehmetoglu, E.
Kasliwal, M. M.
Kirshner, R. P.
Krisciunas, K.
Kumar, S.
Lu, J.
Marion, G. H.
Mazzali, P. A.
Piro, A. L.
Sand, D. J.
Stritzinger, M. D.
Suntzeff, N. B.
Taddia, F.
Uddin, S. A.
author2_role author
author
author
author
author
author
author
author
author
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 SUPERNOVAE
topic SUPERNOVAE
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 75 near-infrared (NIR; 0.8-2.5 μm) spectra of 34 stripped-envelope core-collapse supernovae (SESNe) obtained by the Carnegie Supernova Project-II (CSP-II), encompassing optical spectroscopic Types IIb, Ib, Ic, and Ic-BL. The spectra range in phase from pre-maximum to 80 days past maximum. This unique data set constitutes the largest NIR spectroscopic sample of SESNe to date. NIR spectroscopy provides observables with additional information that is not available in the optical. Specifically, the NIR contains the strong lines of He i and allows a more detailed look at whether Type Ic supernovae are completely stripped of their outer He layer. The NIR spectra of SESNe have broad similarities, but closer examination through statistical means reveals a strong dichotomy between NIR "He-rich"and "He-poor"SNe. These NIR subgroups correspond almost perfectly to the optical IIb/Ib and Ic/Ic-BL types, respectively. The largest difference between the two groups is observed in the 2 μm region, near the He i λ2.0581 μm line. The division between the two groups is not an arbitrary one along a continuous sequence. Early spectra of He-rich SESNe show much stronger He i λ2.0581 μm absorption compared to the He-poor group, but with a wide range of profile shapes. The same line also provides evidence for trace amounts of He in half of our SNe in the He-poor group.
Fil: Shahbandeh, M.. Florida State University; Estados Unidos
Fil: Hsiao, E. Y.. Florida State University; Estados Unidos
Fil: Ashall, C.. University Hawaii Institute For Astronomy; Estados Unidos
Fil: Teffs, J.. Liverpool John Moores University; Reino Unido
Fil: Hoeflich, P.. Florida State University; Estados Unidos
Fil: Morrell, N.. Las Campanas Observatory; Chile
Fil: Phillips, M. M.. Las Campanas Observatory; Chile
Fil: Anderson, J. P.. European Southern Observatory Santiago; Chile
Fil: Baron, E.. No especifíca;
Fil: Burns, C. R.. No especifíca;
Fil: Contreras, C.. Las Campanas Observatory; Chile
Fil: Davis, S.. University of California at Davis; Estados Unidos
Fil: Diamond, T. R.. Private Astronomer; Estados Unidos
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: Galbany, L.. Consejo Superior de Investigaciones Científicas; España
Fil: Gall, C.. No especifíca;
Fil: Hachinger, S.. No especifíca;
Fil: Holmbo, S.. University Aarhus; Dinamarca
Fil: Karamehmetoglu, E.. University Aarhus; Dinamarca
Fil: Kasliwal, M. M.. California Institute of Technology; Estados Unidos
Fil: Kirshner, R. P.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Krisciunas, K.. Texas A&M University; Estados Unidos
Fil: Kumar, S.. Florida State University; Estados Unidos
Fil: Lu, J.. Florida State University; Estados Unidos
Fil: Marion, G. H.. University of Texas at Austin; Estados Unidos
Fil: Mazzali, P. A.. Gobierno de la República Federal de Alemania. Max Planck Institut für Astrophysik; Alemania
Fil: Piro, A. L.. No especifíca;
Fil: Sand, D. J.. University of Arizona; Estados Unidos
Fil: Stritzinger, M. D.. University Aarhus; Dinamarca
Fil: Suntzeff, N. B.. Texas A&M University; Estados Unidos
Fil: Taddia, F.. University Aarhus; Dinamarca
Fil: Uddin, S. A.. Texas A&M University; Estados Unidos
description We present 75 near-infrared (NIR; 0.8-2.5 μm) spectra of 34 stripped-envelope core-collapse supernovae (SESNe) obtained by the Carnegie Supernova Project-II (CSP-II), encompassing optical spectroscopic Types IIb, Ib, Ic, and Ic-BL. The spectra range in phase from pre-maximum to 80 days past maximum. This unique data set constitutes the largest NIR spectroscopic sample of SESNe to date. NIR spectroscopy provides observables with additional information that is not available in the optical. Specifically, the NIR contains the strong lines of He i and allows a more detailed look at whether Type Ic supernovae are completely stripped of their outer He layer. The NIR spectra of SESNe have broad similarities, but closer examination through statistical means reveals a strong dichotomy between NIR "He-rich"and "He-poor"SNe. These NIR subgroups correspond almost perfectly to the optical IIb/Ib and Ic/Ic-BL types, respectively. The largest difference between the two groups is observed in the 2 μm region, near the He i λ2.0581 μm line. The division between the two groups is not an arbitrary one along a continuous sequence. Early spectra of He-rich SESNe show much stronger He i λ2.0581 μm absorption compared to the He-poor group, but with a wide range of profile shapes. The same line also provides evidence for trace amounts of He in half of our SNe in the He-poor group.
publishDate 2022
dc.date.none.fl_str_mv 2022-02
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/11336/210879
Shahbandeh, M.; Hsiao, E. Y.; Ashall, C.; Teffs, J.; Hoeflich, P.; et al.; Carnegie Supernova Project-II: Near-infrared Spectroscopy of Stripped-envelope Core-collapse Supernovae; IOP Publishing; Astrophysical Journal; 925; 2; 2-2022; 1-24
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/210879
identifier_str_mv Shahbandeh, M.; Hsiao, E. Y.; Ashall, C.; Teffs, J.; Hoeflich, P.; et al.; Carnegie Supernova Project-II: Near-infrared Spectroscopy of Stripped-envelope Core-collapse Supernovae; IOP Publishing; Astrophysical Journal; 925; 2; 2-2022; 1-24
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/ac4030
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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