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
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/210879
Ver los metadatos del registro completo
| id |
CONICETDig_d215b4a8b6a84ebfdd4e500d00dbb462 |
|---|---|
| oai_identifier_str |
oai:ri.conicet.gov.ar:11336/210879 |
| network_acronym_str |
CONICETDig |
| repository_id_str |
3498 |
| 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 Técnicas2025-10-22T11:08:00Zoai: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:34982025-10-22 11:08:00.53CONICET 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 |
| _version_ |
1846781404099117056 |
| score |
12.982451 |