The Carnegie Supernova Project I : Third Photometry Data Release of Low-redshift Type Ia Supernovae and Other White Dwarf Explosions
- Autores
- Krisciunas, K.; Contreras, Carlos; Burns, Christopher R.; Phillips, Mark M.; Hamuy, Mario; Stritzinger, Maximilian; Anais, J.; Boldt, Luis; Busta, Luis; Campillay, Abdo; Castellon, S.; Folatelli, Gastón; Freedman, Wendy L.; González, Consuelo; Hsiao, Eric Y.; Krzeminski, Wojtek; Morrell, Nidia Irene; Persson, S. E.; Roth, M.; Salgado, Francisco; Serón, Jacqueline; Suntzeff, Nicholas B.; Torres, Simón; Filippenko, Alexei V.; Li, Weidong; Madore, Barry F.; Depoy, D. L.; Marshall, J. L.; Rheault, J. P.; Villanueva, Steven
- Año de publicación
- 2017
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present final natural-system optical (ugriBV) and near-infrared (YJH) photometry of 134 supernovae (SNe) with probable white dwarf progenitors that were observed in 2004-2009 as part of the first stage of the Carnegie Supernova Project (CSP-I). The sample consists of 123 Type Ia SNe, 5 Type Iax SNe, 2 super-Chandrasekhar SN candidates, 2 Type Ia SNe interacting with circumstellar matter, and 2 SN 2006bt-like events. The redshifts of the objects range from to 0.0835; the median redshift is 0.0241. For 120 (90%) of these SNe, near-infrared photometry was obtained. Average optical extinction coefficients and color terms are derived and demonstrated to be stable during the five CSP-I observing campaigns. Measurements of the CSP-I near-infrared bandpasses are also described, and near-infrared color terms are estimated through synthetic photometry of stellar atmosphere models. Optical and near-infrared magnitudes of local sequences of tertiary standard stars for each supernova are given, and a new calibration of Y-band magnitudes of the Persson et al. standards in the CSP-I natural system is presented.
Este trabajo tiene una errata (ver "Documentos relacionados").
Facultad de Ciencias Astronómicas y Geofísicas
Instituto de Astrofísica de La Plata - Materia
-
Ciencias Astronómicas
instrumentation: photometers
supernovae: general
surveys
techniques: photometric - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by/3.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/87213
Ver los metadatos del registro completo
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The Carnegie Supernova Project I : Third Photometry Data Release of Low-redshift Type Ia Supernovae and Other White Dwarf ExplosionsKrisciunas, K.Contreras, CarlosBurns, Christopher R.Phillips, Mark M.Hamuy, MarioStritzinger, MaximilianAnais, J.Boldt, LuisBusta, LuisCampillay, AbdoCastellon, S.Folatelli, GastónFreedman, Wendy L.González, ConsueloHsiao, Eric Y.Krzeminski, WojtekMorrell, Nidia IrenePersson, S. E.Roth, M.Salgado, FranciscoSerón, JacquelineSuntzeff, Nicholas B.Torres, SimónFilippenko, Alexei V.Li, WeidongMadore, Barry F.Depoy, D. L.Marshall, J. L.Rheault, J. P.Villanueva, StevenCiencias Astronómicasinstrumentation: photometerssupernovae: generalsurveystechniques: photometricWe present final natural-system optical (<i>ugriBV</i>) and near-infrared (<i>YJH</i>) photometry of 134 supernovae (SNe) with probable white dwarf progenitors that were observed in 2004-2009 as part of the first stage of the Carnegie Supernova Project (CSP-I). The sample consists of 123 Type Ia SNe, 5 Type Iax SNe, 2 super-Chandrasekhar SN candidates, 2 Type Ia SNe interacting with circumstellar matter, and 2 SN 2006bt-like events. The redshifts of the objects range from to 0.0835; the median redshift is 0.0241. For 120 (90%) of these SNe, near-infrared photometry was obtained. Average optical extinction coefficients and color terms are derived and demonstrated to be stable during the five CSP-I observing campaigns. Measurements of the CSP-I near-infrared bandpasses are also described, and near-infrared color terms are estimated through synthetic photometry of stellar atmosphere models. Optical and near-infrared magnitudes of local sequences of tertiary standard stars for each supernova are given, and a new calibration of Y-band magnitudes of the Persson et al. standards in the CSP-I natural system is presented.Este trabajo tiene una errata (ver "Documentos relacionados").Facultad de Ciencias Astronómicas y GeofísicasInstituto de Astrofísica de La Plata2017info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/87213enginfo:eu-repo/semantics/altIdentifier/issn/0004-6256info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-3881/aa8df0info:eu-repo/semantics/reference/hdl/10915/135592info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/3.0/Creative Commons Attribution 3.0 Unported (CC BY 3.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:17:09Zoai:sedici.unlp.edu.ar:10915/87213Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:17:10.275SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
The Carnegie Supernova Project I : Third Photometry Data Release of Low-redshift Type Ia Supernovae and Other White Dwarf Explosions |
title |
The Carnegie Supernova Project I : Third Photometry Data Release of Low-redshift Type Ia Supernovae and Other White Dwarf Explosions |
spellingShingle |
The Carnegie Supernova Project I : Third Photometry Data Release of Low-redshift Type Ia Supernovae and Other White Dwarf Explosions Krisciunas, K. Ciencias Astronómicas instrumentation: photometers supernovae: general surveys techniques: photometric |
title_short |
The Carnegie Supernova Project I : Third Photometry Data Release of Low-redshift Type Ia Supernovae and Other White Dwarf Explosions |
title_full |
The Carnegie Supernova Project I : Third Photometry Data Release of Low-redshift Type Ia Supernovae and Other White Dwarf Explosions |
title_fullStr |
The Carnegie Supernova Project I : Third Photometry Data Release of Low-redshift Type Ia Supernovae and Other White Dwarf Explosions |
title_full_unstemmed |
The Carnegie Supernova Project I : Third Photometry Data Release of Low-redshift Type Ia Supernovae and Other White Dwarf Explosions |
title_sort |
The Carnegie Supernova Project I : Third Photometry Data Release of Low-redshift Type Ia Supernovae and Other White Dwarf Explosions |
dc.creator.none.fl_str_mv |
Krisciunas, K. Contreras, Carlos Burns, Christopher R. Phillips, Mark M. Hamuy, Mario Stritzinger, Maximilian Anais, J. Boldt, Luis Busta, Luis Campillay, Abdo Castellon, S. Folatelli, Gastón Freedman, Wendy L. González, Consuelo Hsiao, Eric Y. Krzeminski, Wojtek Morrell, Nidia Irene Persson, S. E. Roth, M. Salgado, Francisco Serón, Jacqueline Suntzeff, Nicholas B. Torres, Simón Filippenko, Alexei V. Li, Weidong Madore, Barry F. Depoy, D. L. Marshall, J. L. Rheault, J. P. Villanueva, Steven |
author |
Krisciunas, K. |
author_facet |
Krisciunas, K. Contreras, Carlos Burns, Christopher R. Phillips, Mark M. Hamuy, Mario Stritzinger, Maximilian Anais, J. Boldt, Luis Busta, Luis Campillay, Abdo Castellon, S. Folatelli, Gastón Freedman, Wendy L. González, Consuelo Hsiao, Eric Y. Krzeminski, Wojtek Morrell, Nidia Irene Persson, S. E. Roth, M. Salgado, Francisco Serón, Jacqueline Suntzeff, Nicholas B. Torres, Simón Filippenko, Alexei V. Li, Weidong Madore, Barry F. Depoy, D. L. Marshall, J. L. Rheault, J. P. Villanueva, Steven |
author_role |
author |
author2 |
Contreras, Carlos Burns, Christopher R. Phillips, Mark M. Hamuy, Mario Stritzinger, Maximilian Anais, J. Boldt, Luis Busta, Luis Campillay, Abdo Castellon, S. Folatelli, Gastón Freedman, Wendy L. González, Consuelo Hsiao, Eric Y. Krzeminski, Wojtek Morrell, Nidia Irene Persson, S. E. Roth, M. Salgado, Francisco Serón, Jacqueline Suntzeff, Nicholas B. Torres, Simón Filippenko, Alexei V. Li, Weidong Madore, Barry F. Depoy, D. L. Marshall, J. L. Rheault, J. P. Villanueva, Steven |
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 |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas instrumentation: photometers supernovae: general surveys techniques: photometric |
topic |
Ciencias Astronómicas instrumentation: photometers supernovae: general surveys techniques: photometric |
dc.description.none.fl_txt_mv |
We present final natural-system optical (<i>ugriBV</i>) and near-infrared (<i>YJH</i>) photometry of 134 supernovae (SNe) with probable white dwarf progenitors that were observed in 2004-2009 as part of the first stage of the Carnegie Supernova Project (CSP-I). The sample consists of 123 Type Ia SNe, 5 Type Iax SNe, 2 super-Chandrasekhar SN candidates, 2 Type Ia SNe interacting with circumstellar matter, and 2 SN 2006bt-like events. The redshifts of the objects range from to 0.0835; the median redshift is 0.0241. For 120 (90%) of these SNe, near-infrared photometry was obtained. Average optical extinction coefficients and color terms are derived and demonstrated to be stable during the five CSP-I observing campaigns. Measurements of the CSP-I near-infrared bandpasses are also described, and near-infrared color terms are estimated through synthetic photometry of stellar atmosphere models. Optical and near-infrared magnitudes of local sequences of tertiary standard stars for each supernova are given, and a new calibration of Y-band magnitudes of the Persson et al. standards in the CSP-I natural system is presented. Este trabajo tiene una errata (ver "Documentos relacionados"). Facultad de Ciencias Astronómicas y Geofísicas Instituto de Astrofísica de La Plata |
description |
We present final natural-system optical (<i>ugriBV</i>) and near-infrared (<i>YJH</i>) photometry of 134 supernovae (SNe) with probable white dwarf progenitors that were observed in 2004-2009 as part of the first stage of the Carnegie Supernova Project (CSP-I). The sample consists of 123 Type Ia SNe, 5 Type Iax SNe, 2 super-Chandrasekhar SN candidates, 2 Type Ia SNe interacting with circumstellar matter, and 2 SN 2006bt-like events. The redshifts of the objects range from to 0.0835; the median redshift is 0.0241. For 120 (90%) of these SNe, near-infrared photometry was obtained. Average optical extinction coefficients and color terms are derived and demonstrated to be stable during the five CSP-I observing campaigns. Measurements of the CSP-I near-infrared bandpasses are also described, and near-infrared color terms are estimated through synthetic photometry of stellar atmosphere models. Optical and near-infrared magnitudes of local sequences of tertiary standard stars for each supernova are given, and a new calibration of Y-band magnitudes of the Persson et al. standards in the CSP-I natural system is presented. |
publishDate |
2017 |
dc.date.none.fl_str_mv |
2017 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo 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://sedici.unlp.edu.ar/handle/10915/87213 |
url |
http://sedici.unlp.edu.ar/handle/10915/87213 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/issn/0004-6256 info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-3881/aa8df0 info:eu-repo/semantics/reference/hdl/10915/135592 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/3.0/ Creative Commons Attribution 3.0 Unported (CC BY 3.0) |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
http://creativecommons.org/licenses/by/3.0/ Creative Commons Attribution 3.0 Unported (CC BY 3.0) |
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application/pdf |
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