Carnegie Supernova Project I and II: Measurements of H 0 Using Cepheid, Tip of the Red Giant Branch, and Surface Brightness Fluctuation Distance Calibration to Type Ia Supernovae

Autores: Uddin, Syed A.; Burns, Christopher R.; Phillips, M. M.; Suntzeff, Nicholas B.; Freedman, Wendy L.; Folatelli, Gaston; Morrell, Nidia Irene; Galbany, Lluís; Kumar, Sahana; Shahbandeh, Melissa; Davis, Scott; Anais, Jorge; Busta, Luis; Campillay, Abdo; Castellón, Sergio; Corco, Carlos; Diamond, Tiara; Gall, Christa; Gonzalez, Consuelo; Holmbo, Simon; Roth, Miguel; Serón, Jacqueline; Taddia, Francesco; Torres, Simón; Baltay, Charles; Hadjiyska, Ellie; Kasliwal, Mansi; Folatelli, Gaston; Nugent, Peter E.; Rabinowitz, David; Ryder, Stuart D.
Año de publicación: 2024
Idioma: inglés
Tipo de recurso: artículo
Estado: versión publicada
Descripción: We present an analysis of Type Ia supernovae (SNe Ia) from the Carnegie Supernova Project I and II and extend the Hubble diagram from optical to near-infrared wavelengths (uBgVriYJH). We calculate the Hubble constant, H0, using various distance calibrators: Cepheids, the tip of the red giant branch (TRGB), and surface brightness fluctuations (SBFs). Combining all methods of calibration, we derive H0 = 71.76 ± 0.58 (stat) ± 1.19 (sys) km s−1 Mpc−1 from the B band and H0 = 73.22 ± 0.68 (stat) ± 1.28 (sys) km s−1 Mpc−1 from the H band. By assigning equal weight to the Cepheid, TRGB, and SBF calibrators, we derive the systematic errors required for consistency in the first rung of the distance ladder, resulting in a systematic error of 1.2 ∼ 1.3 km s−1 Mpc−1 in H0. As a result, relative to the statistics-only uncertainty, the tension between the late-time H0 we derive by combining the various distance calibrators and the early-time H0 from the cosmic microwave background is reduced. The highest precision in SN Ia luminosity is found in the Y band (0.12 ± 0.01 mag), as defined by the intrinsic scatter (σint). We revisit SN Ia Hubble residual-host mass correlations and recover previous results that these correlations do not change significantly between the optical and near-infrared wavelengths. Finally, SNe Ia that explode beyond 10 kpc from their host centers exhibit smaller dispersion in their luminosity, confirming our earlier findings. A reduced effect of dust in the outskirts of hosts may be responsible for this effect.
Fil: Uddin, Syed A.. Observatories of the Carnegie Institution for Science; Estados Unidos
Fil: Burns, Christopher R.. Observatories of the Carnegie Institution for Science; Estados Unidos
Fil: Phillips, M. M.. Las Campanas Observatory; Chile
Fil: Suntzeff, Nicholas B.. Texas A&M University; Estados Unidos
Fil: Freedman, Wendy L.. University of Chicago; 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: Morrell, Nidia Irene. Las Campanas Observatory; Chile. 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, Lluís. Institute of Space Sciences; España
Fil: Kumar, Sahana. Florida State University; Estados Unidos
Fil: Shahbandeh, Melissa. Johns Hopkins University; Estados Unidos
Fil: Davis, Scott. University of California; Estados Unidos
Fil: Anais, Jorge. Universidad de Antofagasta;
Fil: Busta, Luis. Las Campanas Observatory; Chile
Fil: Campillay, Abdo. Las Campanas Observatory; Chile
Fil: Castellón, Sergio. Las Campanas Observatory; Chile
Fil: Corco, Carlos. Las Campanas Observatory; Chile
Fil: Diamond, Tiara. Florida State University; Estados Unidos
Fil: Gall, Christa. University of Copenhagen; Dinamarca
Fil: Gonzalez, Consuelo. Las Camapanas Observatory; Chile
Fil: Holmbo, Simon. Aarhus University; Dinamarca
Fil: Roth, Miguel. Las Camapanas Observatory; Chile
Fil: Serón, Jacqueline. Cerro Tololo Inter-American Observatory; Chile
Fil: Taddia, Francesco. Stockholm University; Suecia
Fil: Torres, Simón. SOAR Telescope; Chile
Fil: Baltay, Charles. Yale University; Estados Unidos
Fil: Hadjiyska, Ellie. Yale University; Estados Unidos
Fil: Kasliwal, Mansi. California Institute of Technology; 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: Nugent, Peter E.. Lawrence Berkeley National Laboratory; Estados Unidos
Fil: Rabinowitz, David. Yale University; Estados Unidos
Fil: Ryder, Stuart D.. Macquarie University; Australia
Materia: Supernovae
Cosmology
Nivel de accesibilidad: acceso abierto
Condiciones de uso: https://creativecommons.org/licenses/by/2.5/ar/
Repositorio
Institución: Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador: oai:ri.conicet.gov.ar:11336/258857

Acceder

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repository_id_str	3498
network_name_str	CONICET Digital (CONICET)
spelling	Carnegie Supernova Project I and II: Measurements of H 0 Using Cepheid, Tip of the Red Giant Branch, and Surface Brightness Fluctuation Distance Calibration to Type Ia SupernovaeUddin, Syed A.Burns, Christopher R.Phillips, M. M.Suntzeff, Nicholas B.Freedman, Wendy L.Folatelli, GastonMorrell, Nidia IreneGalbany, LluísKumar, SahanaShahbandeh, MelissaDavis, ScottAnais, JorgeBusta, LuisCampillay, AbdoCastellón, SergioCorco, CarlosDiamond, TiaraGall, ChristaGonzalez, ConsueloHolmbo, SimonRoth, MiguelSerón, JacquelineTaddia, FrancescoTorres, SimónBaltay, CharlesHadjiyska, EllieKasliwal, MansiFolatelli, GastonNugent, Peter E.Rabinowitz, DavidRyder, Stuart D.SupernovaeCosmologyhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present an analysis of Type Ia supernovae (SNe Ia) from the Carnegie Supernova Project I and II and extend the Hubble diagram from optical to near-infrared wavelengths (uBgVriYJH). We calculate the Hubble constant, H0, using various distance calibrators: Cepheids, the tip of the red giant branch (TRGB), and surface brightness fluctuations (SBFs). Combining all methods of calibration, we derive H0 = 71.76 ± 0.58 (stat) ± 1.19 (sys) km s−1 Mpc−1 from the B band and H0 = 73.22 ± 0.68 (stat) ± 1.28 (sys) km s−1 Mpc−1 from the H band. By assigning equal weight to the Cepheid, TRGB, and SBF calibrators, we derive the systematic errors required for consistency in the first rung of the distance ladder, resulting in a systematic error of 1.2 ∼ 1.3 km s−1 Mpc−1 in H0. As a result, relative to the statistics-only uncertainty, the tension between the late-time H0 we derive by combining the various distance calibrators and the early-time H0 from the cosmic microwave background is reduced. The highest precision in SN Ia luminosity is found in the Y band (0.12 ± 0.01 mag), as defined by the intrinsic scatter (σint). We revisit SN Ia Hubble residual-host mass correlations and recover previous results that these correlations do not change significantly between the optical and near-infrared wavelengths. Finally, SNe Ia that explode beyond 10 kpc from their host centers exhibit smaller dispersion in their luminosity, confirming our earlier findings. A reduced effect of dust in the outskirts of hosts may be responsible for this effect.Fil: Uddin, Syed A.. Observatories of the Carnegie Institution for Science; Estados UnidosFil: Burns, Christopher R.. Observatories of the Carnegie Institution for Science; Estados UnidosFil: Phillips, M. M.. Las Campanas Observatory; ChileFil: Suntzeff, Nicholas B.. Texas A&M University; Estados UnidosFil: Freedman, Wendy L.. University of Chicago; 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: Morrell, Nidia Irene. Las Campanas Observatory; Chile. 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, Lluís. Institute of Space Sciences; EspañaFil: Kumar, Sahana. Florida State University; Estados UnidosFil: Shahbandeh, Melissa. Johns Hopkins University; Estados UnidosFil: Davis, Scott. University of California; Estados UnidosFil: Anais, Jorge. Universidad de Antofagasta;Fil: Busta, Luis. Las Campanas Observatory; ChileFil: Campillay, Abdo. Las Campanas Observatory; ChileFil: Castellón, Sergio. Las Campanas Observatory; ChileFil: Corco, Carlos. Las Campanas Observatory; ChileFil: Diamond, Tiara. Florida State University; Estados UnidosFil: Gall, Christa. University of Copenhagen; DinamarcaFil: Gonzalez, Consuelo. Las Camapanas Observatory; ChileFil: Holmbo, Simon. Aarhus University; DinamarcaFil: Roth, Miguel. Las Camapanas Observatory; ChileFil: Serón, Jacqueline. Cerro Tololo Inter-American Observatory; ChileFil: Taddia, Francesco. Stockholm University; SueciaFil: Torres, Simón. SOAR Telescope; ChileFil: Baltay, Charles. Yale University; Estados UnidosFil: Hadjiyska, Ellie. Yale University; Estados UnidosFil: Kasliwal, Mansi. California Institute of Technology; 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: Nugent, Peter E.. Lawrence Berkeley National Laboratory; Estados UnidosFil: Rabinowitz, David. Yale University; Estados UnidosFil: Ryder, Stuart D.. Macquarie University; AustraliaIOP Publishing2024-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/258857Uddin, Syed A.; Burns, Christopher R.; Phillips, M. M.; Suntzeff, Nicholas B.; Freedman, Wendy L.; et al.; Carnegie Supernova Project I and II: Measurements of H 0 Using Cepheid, Tip of the Red Giant Branch, and Surface Brightness Fluctuation Distance Calibration to Type Ia Supernovae; IOP Publishing; Astrophysical Journal; 970; 1; 7-2024; 72; 1-290004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/ad3e63info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ad3e63info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:44:48Zoai:ri.conicet.gov.ar:11336/258857instacron: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 09:44:49.145CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv	Carnegie Supernova Project I and II: Measurements of H 0 Using Cepheid, Tip of the Red Giant Branch, and Surface Brightness Fluctuation Distance Calibration to Type Ia Supernovae
title	Carnegie Supernova Project I and II: Measurements of H 0 Using Cepheid, Tip of the Red Giant Branch, and Surface Brightness Fluctuation Distance Calibration to Type Ia Supernovae
spellingShingle	Carnegie Supernova Project I and II: Measurements of H 0 Using Cepheid, Tip of the Red Giant Branch, and Surface Brightness Fluctuation Distance Calibration to Type Ia Supernovae Uddin, Syed A. Supernovae Cosmology
title_short	Carnegie Supernova Project I and II: Measurements of H 0 Using Cepheid, Tip of the Red Giant Branch, and Surface Brightness Fluctuation Distance Calibration to Type Ia Supernovae
title_full	Carnegie Supernova Project I and II: Measurements of H 0 Using Cepheid, Tip of the Red Giant Branch, and Surface Brightness Fluctuation Distance Calibration to Type Ia Supernovae
title_fullStr	Carnegie Supernova Project I and II: Measurements of H 0 Using Cepheid, Tip of the Red Giant Branch, and Surface Brightness Fluctuation Distance Calibration to Type Ia Supernovae
title_full_unstemmed	Carnegie Supernova Project I and II: Measurements of H 0 Using Cepheid, Tip of the Red Giant Branch, and Surface Brightness Fluctuation Distance Calibration to Type Ia Supernovae
title_sort	Carnegie Supernova Project I and II: Measurements of H 0 Using Cepheid, Tip of the Red Giant Branch, and Surface Brightness Fluctuation Distance Calibration to Type Ia Supernovae
dc.creator.none.fl_str_mv	Uddin, Syed A. Burns, Christopher R. Phillips, M. M. Suntzeff, Nicholas B. Freedman, Wendy L. Folatelli, Gaston Morrell, Nidia Irene Galbany, Lluís Kumar, Sahana Shahbandeh, Melissa Davis, Scott Anais, Jorge Busta, Luis Campillay, Abdo Castellón, Sergio Corco, Carlos Diamond, Tiara Gall, Christa Gonzalez, Consuelo Holmbo, Simon Roth, Miguel Serón, Jacqueline Taddia, Francesco Torres, Simón Baltay, Charles Hadjiyska, Ellie Kasliwal, Mansi Folatelli, Gaston Nugent, Peter E. Rabinowitz, David Ryder, Stuart D.
author	Uddin, Syed A.
author_facet	Uddin, Syed A. Burns, Christopher R. Phillips, M. M. Suntzeff, Nicholas B. Freedman, Wendy L. Folatelli, Gaston Morrell, Nidia Irene Galbany, Lluís Kumar, Sahana Shahbandeh, Melissa Davis, Scott Anais, Jorge Busta, Luis Campillay, Abdo Castellón, Sergio Corco, Carlos Diamond, Tiara Gall, Christa Gonzalez, Consuelo Holmbo, Simon Roth, Miguel Serón, Jacqueline Taddia, Francesco Torres, Simón Baltay, Charles Hadjiyska, Ellie Kasliwal, Mansi Nugent, Peter E. Rabinowitz, David Ryder, Stuart D.
author_role	author
author2	Burns, Christopher R. Phillips, M. M. Suntzeff, Nicholas B. Freedman, Wendy L. Folatelli, Gaston Morrell, Nidia Irene Galbany, Lluís Kumar, Sahana Shahbandeh, Melissa Davis, Scott Anais, Jorge Busta, Luis Campillay, Abdo Castellón, Sergio Corco, Carlos Diamond, Tiara Gall, Christa Gonzalez, Consuelo Holmbo, Simon Roth, Miguel Serón, Jacqueline Taddia, Francesco Torres, Simón Baltay, Charles Hadjiyska, Ellie Kasliwal, Mansi Nugent, Peter E. Rabinowitz, David Ryder, Stuart D.
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	Supernovae Cosmology
topic	Supernovae Cosmology
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 an analysis of Type Ia supernovae (SNe Ia) from the Carnegie Supernova Project I and II and extend the Hubble diagram from optical to near-infrared wavelengths (uBgVriYJH). We calculate the Hubble constant, H0, using various distance calibrators: Cepheids, the tip of the red giant branch (TRGB), and surface brightness fluctuations (SBFs). Combining all methods of calibration, we derive H0 = 71.76 ± 0.58 (stat) ± 1.19 (sys) km s−1 Mpc−1 from the B band and H0 = 73.22 ± 0.68 (stat) ± 1.28 (sys) km s−1 Mpc−1 from the H band. By assigning equal weight to the Cepheid, TRGB, and SBF calibrators, we derive the systematic errors required for consistency in the first rung of the distance ladder, resulting in a systematic error of 1.2 ∼ 1.3 km s−1 Mpc−1 in H0. As a result, relative to the statistics-only uncertainty, the tension between the late-time H0 we derive by combining the various distance calibrators and the early-time H0 from the cosmic microwave background is reduced. The highest precision in SN Ia luminosity is found in the Y band (0.12 ± 0.01 mag), as defined by the intrinsic scatter (σint). We revisit SN Ia Hubble residual-host mass correlations and recover previous results that these correlations do not change significantly between the optical and near-infrared wavelengths. Finally, SNe Ia that explode beyond 10 kpc from their host centers exhibit smaller dispersion in their luminosity, confirming our earlier findings. A reduced effect of dust in the outskirts of hosts may be responsible for this effect. Fil: Uddin, Syed A.. Observatories of the Carnegie Institution for Science; Estados Unidos Fil: Burns, Christopher R.. Observatories of the Carnegie Institution for Science; Estados Unidos Fil: Phillips, M. M.. Las Campanas Observatory; Chile Fil: Suntzeff, Nicholas B.. Texas A&M University; Estados Unidos Fil: Freedman, Wendy L.. University of Chicago; 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: Morrell, Nidia Irene. Las Campanas Observatory; Chile. 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, Lluís. Institute of Space Sciences; España Fil: Kumar, Sahana. Florida State University; Estados Unidos Fil: Shahbandeh, Melissa. Johns Hopkins University; Estados Unidos Fil: Davis, Scott. University of California; Estados Unidos Fil: Anais, Jorge. Universidad de Antofagasta; Fil: Busta, Luis. Las Campanas Observatory; Chile Fil: Campillay, Abdo. Las Campanas Observatory; Chile Fil: Castellón, Sergio. Las Campanas Observatory; Chile Fil: Corco, Carlos. Las Campanas Observatory; Chile Fil: Diamond, Tiara. Florida State University; Estados Unidos Fil: Gall, Christa. University of Copenhagen; Dinamarca Fil: Gonzalez, Consuelo. Las Camapanas Observatory; Chile Fil: Holmbo, Simon. Aarhus University; Dinamarca Fil: Roth, Miguel. Las Camapanas Observatory; Chile Fil: Serón, Jacqueline. Cerro Tololo Inter-American Observatory; Chile Fil: Taddia, Francesco. Stockholm University; Suecia Fil: Torres, Simón. SOAR Telescope; Chile Fil: Baltay, Charles. Yale University; Estados Unidos Fil: Hadjiyska, Ellie. Yale University; Estados Unidos Fil: Kasliwal, Mansi. California Institute of Technology; 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: Nugent, Peter E.. Lawrence Berkeley National Laboratory; Estados Unidos Fil: Rabinowitz, David. Yale University; Estados Unidos Fil: Ryder, Stuart D.. Macquarie University; Australia
description	We present an analysis of Type Ia supernovae (SNe Ia) from the Carnegie Supernova Project I and II and extend the Hubble diagram from optical to near-infrared wavelengths (uBgVriYJH). We calculate the Hubble constant, H0, using various distance calibrators: Cepheids, the tip of the red giant branch (TRGB), and surface brightness fluctuations (SBFs). Combining all methods of calibration, we derive H0 = 71.76 ± 0.58 (stat) ± 1.19 (sys) km s−1 Mpc−1 from the B band and H0 = 73.22 ± 0.68 (stat) ± 1.28 (sys) km s−1 Mpc−1 from the H band. By assigning equal weight to the Cepheid, TRGB, and SBF calibrators, we derive the systematic errors required for consistency in the first rung of the distance ladder, resulting in a systematic error of 1.2 ∼ 1.3 km s−1 Mpc−1 in H0. As a result, relative to the statistics-only uncertainty, the tension between the late-time H0 we derive by combining the various distance calibrators and the early-time H0 from the cosmic microwave background is reduced. The highest precision in SN Ia luminosity is found in the Y band (0.12 ± 0.01 mag), as defined by the intrinsic scatter (σint). We revisit SN Ia Hubble residual-host mass correlations and recover previous results that these correlations do not change significantly between the optical and near-infrared wavelengths. Finally, SNe Ia that explode beyond 10 kpc from their host centers exhibit smaller dispersion in their luminosity, confirming our earlier findings. A reduced effect of dust in the outskirts of hosts may be responsible for this effect.
publishDate	2024
dc.date.none.fl_str_mv	2024-07
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/11336/258857 Uddin, Syed A.; Burns, Christopher R.; Phillips, M. M.; Suntzeff, Nicholas B.; Freedman, Wendy L.; et al.; Carnegie Supernova Project I and II: Measurements of H 0 Using Cepheid, Tip of the Red Giant Branch, and Surface Brightness Fluctuation Distance Calibration to Type Ia Supernovae; IOP Publishing; Astrophysical Journal; 970; 1; 7-2024; 72; 1-29 0004-637X CONICET Digital CONICET
url	http://hdl.handle.net/11336/258857
identifier_str_mv	Uddin, Syed A.; Burns, Christopher R.; Phillips, M. M.; Suntzeff, Nicholas B.; Freedman, Wendy L.; et al.; Carnegie Supernova Project I and II: Measurements of H 0 Using Cepheid, Tip of the Red Giant Branch, and Surface Brightness Fluctuation Distance Calibration to Type Ia Supernovae; IOP Publishing; Astrophysical Journal; 970; 1; 7-2024; 72; 1-29 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/url/https://iopscience.iop.org/article/10.3847/1538-4357/ad3e63 info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ad3e63
dc.rights.none.fl_str_mv	info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by/2.5/ar/
eu_rights_str_mv	openAccess
rights_invalid_str_mv	https://creativecommons.org/licenses/by/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)
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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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Carnegie Supernova Project I and II: Measurements of H 0 Using Cepheid, Tip of the Red Giant Branch, and Surface Brightness Fluctuation Distance Calibration to Type Ia Supernovae

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