The KELT Follow-up Network and Transit False-positive Catalog: Pre-vetted False Positives for TESS

Autores
Collins, Karen A.; Collins, Kevin I.; Pepper, Joshua; Labadie Bartz, Jonathan; Stassun, Keivan G.; Gaudi, B. Scott; Bayliss, Daniel; Bento, Joao; Colón, Knicole D.; Feliz, Dax; James, David; Johnson, Marshall C.; Kuhn, Rudolf B.; Lund, Michael B.; Penny, Matthew T.; Rodriguez, Joseph E.; Siverd, Robert J.; Stevens, Daniel J.; Yao, Xinyu; Zhou, George; Akshay, Mundra; Aldi, Giulio F.; Ashcraft, Cliff; Awiphan, Supachai; Baştürk, Özgür; Baker, David; Beatty, Thomas G.; Benni, Paul; Berlind, Perry; Berriman, Bruce G.; Petrucci, Romina Paola; Jofre, Jorge Emiliano
Año de publicación
2018
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The Kilodegree Extremely Little Telescope (KELT) project has been conducting a photometric survey of transiting planets orbiting bright stars for over 10 years. The KELT images have a pixel scale of ∼23″ pixel-1 - very similar to that of NASA´s Transiting Exoplanet Survey Satellite (TESS) - as well as a large point-spread function, and the KELT reduction pipeline uses a weighted photometric aperture with radius 3′. At this angular scale, multiple stars are typically blended in the photometric apertures. In order to identify false positives and confirm transiting exoplanets, we have assembled a follow-up network (KELT-FUN) to conduct imaging with spatial resolution, cadence, and photometric precision higher than the KELT telescopes, as well as spectroscopic observations of the candidate host stars. The KELT-FUN team has followed-up over 1600 planet candidates since 2011, resulting in more than 20 planet discoveries. Excluding ∼450 false alarms of non-astrophysical origin (i.e., instrumental noise or systematics), we present an all-sky catalog of the 1128 bright stars (6 < V < 13) that show transit-like features in the KELT light curves, but which were subsequently determined to be astrophysical false positives (FPs) after photometric and/or spectroscopic follow-up observations. The KELT-FUN team continues to pursue KELT and other planet candidates and will eventually follow up certain classes of TESS candidates. The KELT FP catalog will help minimize the duplication of follow-up observations by current and future transit surveys such as TESS.
Fil: Collins, Karen A.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Collins, Kevin I.. Vanderbilt University; Estados Unidos
Fil: Pepper, Joshua. Lehigh University; Estados Unidos
Fil: Labadie Bartz, Jonathan. Lehigh University; Estados Unidos. University of Delaware; Estados Unidos
Fil: Stassun, Keivan G.. Fisk University; Estados Unidos. Vanderbilt University; Estados Unidos
Fil: Gaudi, B. Scott. Ohio State University; Estados Unidos
Fil: Bayliss, Daniel. University of Warwick; Reino Unido. Australian National University; Australia
Fil: Bento, Joao. Australian National University; Australia
Fil: Colón, Knicole D.. National Aeronautics and Space Administration; Estados Unidos. Fisk University; Estados Unidos
Fil: Feliz, Dax. Vanderbilt University; Estados Unidos
Fil: James, David. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Johnson, Marshall C.. Ohio State University; Estados Unidos
Fil: Kuhn, Rudolf B.. Southern African Large Telescope; Sudáfrica. South African Astronomical Observatory; Sudáfrica
Fil: Lund, Michael B.. Vanderbilt University; Estados Unidos
Fil: Penny, Matthew T.. Ohio State University; Estados Unidos
Fil: Rodriguez, Joseph E.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Siverd, Robert J.. Las Cumbres Observatory; Estados Unidos
Fil: Stevens, Daniel J.. Ohio State University; Estados Unidos
Fil: Yao, Xinyu. Lehigh University; Estados Unidos
Fil: Zhou, George. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. Australian National University; Australia
Fil: Akshay, Mundra. Phillips Academy; Estados Unidos
Fil: Aldi, Giulio F.. Universita di Salerno; Italia. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Ashcraft, Cliff. Union County College; Estados Unidos
Fil: Awiphan, Supachai. National Astronomical Research Institute of Thailand; Tailandia
Fil: Baştürk, Özgür. Ankara Üniversitesi. Fen Fakültesi; Turquía
Fil: Baker, David. Austin College; Estados Unidos
Fil: Beatty, Thomas G.. State University of Pennsylvania; Estados Unidos
Fil: Benni, Paul. Paul Benni Private Observatory; Estados Unidos
Fil: Berlind, Perry. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Berriman, Bruce G.. State University of Pennsylvania; Estados Unidos
Fil: Petrucci, Romina Paola. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina
Fil: Jofre, Jorge Emiliano. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina
Materia
METHODS: OBSERVATIONAL
TECHNIQUES: PHOTOMETRIC
TECHNIQUES: RADIAL VELOCITIES
TECHNIQUES: SPECTROSCOPIC
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:11336/164440

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network_name_str CONICET Digital (CONICET)
spelling The KELT Follow-up Network and Transit False-positive Catalog: Pre-vetted False Positives for TESSCollins, Karen A.Collins, Kevin I.Pepper, JoshuaLabadie Bartz, JonathanStassun, Keivan G.Gaudi, B. ScottBayliss, DanielBento, JoaoColón, Knicole D.Feliz, DaxJames, DavidJohnson, Marshall C.Kuhn, Rudolf B.Lund, Michael B.Penny, Matthew T.Rodriguez, Joseph E.Siverd, Robert J.Stevens, Daniel J.Yao, XinyuZhou, GeorgeAkshay, MundraAldi, Giulio F.Ashcraft, CliffAwiphan, SupachaiBaştürk, ÖzgürBaker, DavidBeatty, Thomas G.Benni, PaulBerlind, PerryBerriman, Bruce G.Petrucci, Romina PaolaJofre, Jorge EmilianoMETHODS: OBSERVATIONALTECHNIQUES: PHOTOMETRICTECHNIQUES: RADIAL VELOCITIESTECHNIQUES: SPECTROSCOPIChttps://purl.org/becyt/ford/1.7https://purl.org/becyt/ford/1The Kilodegree Extremely Little Telescope (KELT) project has been conducting a photometric survey of transiting planets orbiting bright stars for over 10 years. The KELT images have a pixel scale of ∼23″ pixel-1 - very similar to that of NASA´s Transiting Exoplanet Survey Satellite (TESS) - as well as a large point-spread function, and the KELT reduction pipeline uses a weighted photometric aperture with radius 3′. At this angular scale, multiple stars are typically blended in the photometric apertures. In order to identify false positives and confirm transiting exoplanets, we have assembled a follow-up network (KELT-FUN) to conduct imaging with spatial resolution, cadence, and photometric precision higher than the KELT telescopes, as well as spectroscopic observations of the candidate host stars. The KELT-FUN team has followed-up over 1600 planet candidates since 2011, resulting in more than 20 planet discoveries. Excluding ∼450 false alarms of non-astrophysical origin (i.e., instrumental noise or systematics), we present an all-sky catalog of the 1128 bright stars (6 < V < 13) that show transit-like features in the KELT light curves, but which were subsequently determined to be astrophysical false positives (FPs) after photometric and/or spectroscopic follow-up observations. The KELT-FUN team continues to pursue KELT and other planet candidates and will eventually follow up certain classes of TESS candidates. The KELT FP catalog will help minimize the duplication of follow-up observations by current and future transit surveys such as TESS.Fil: Collins, Karen A.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Collins, Kevin I.. Vanderbilt University; Estados UnidosFil: Pepper, Joshua. Lehigh University; Estados UnidosFil: Labadie Bartz, Jonathan. Lehigh University; Estados Unidos. University of Delaware; Estados UnidosFil: Stassun, Keivan G.. Fisk University; Estados Unidos. Vanderbilt University; Estados UnidosFil: Gaudi, B. Scott. Ohio State University; Estados UnidosFil: Bayliss, Daniel. University of Warwick; Reino Unido. Australian National University; AustraliaFil: Bento, Joao. Australian National University; AustraliaFil: Colón, Knicole D.. National Aeronautics and Space Administration; Estados Unidos. Fisk University; Estados UnidosFil: Feliz, Dax. Vanderbilt University; Estados UnidosFil: James, David. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Johnson, Marshall C.. Ohio State University; Estados UnidosFil: Kuhn, Rudolf B.. Southern African Large Telescope; Sudáfrica. South African Astronomical Observatory; SudáfricaFil: Lund, Michael B.. Vanderbilt University; Estados UnidosFil: Penny, Matthew T.. Ohio State University; Estados UnidosFil: Rodriguez, Joseph E.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Siverd, Robert J.. Las Cumbres Observatory; Estados UnidosFil: Stevens, Daniel J.. Ohio State University; Estados UnidosFil: Yao, Xinyu. Lehigh University; Estados UnidosFil: Zhou, George. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. Australian National University; AustraliaFil: Akshay, Mundra. Phillips Academy; Estados UnidosFil: Aldi, Giulio F.. Universita di Salerno; Italia. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Ashcraft, Cliff. Union County College; Estados UnidosFil: Awiphan, Supachai. National Astronomical Research Institute of Thailand; TailandiaFil: Baştürk, Özgür. Ankara Üniversitesi. Fen Fakültesi; TurquíaFil: Baker, David. Austin College; Estados UnidosFil: Beatty, Thomas G.. State University of Pennsylvania; Estados UnidosFil: Benni, Paul. Paul Benni Private Observatory; Estados UnidosFil: Berlind, Perry. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Berriman, Bruce G.. State University of Pennsylvania; Estados UnidosFil: Petrucci, Romina Paola. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; ArgentinaFil: Jofre, Jorge Emiliano. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; ArgentinaIOP Publishing2018-11info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/164440Collins, Karen A.; Collins, Kevin I.; Pepper, Joshua; Labadie Bartz, Jonathan; Stassun, Keivan G.; et al.; The KELT Follow-up Network and Transit False-positive Catalog: Pre-vetted False Positives for TESS; IOP Publishing; Astronomical Journal; 156; 5; 11-2018; 1-190004-62561538-3881CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-3881/aae582info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-3881/aae582info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:09:05Zoai:ri.conicet.gov.ar:11336/164440instacron: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 10:09:06.052CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The KELT Follow-up Network and Transit False-positive Catalog: Pre-vetted False Positives for TESS
title The KELT Follow-up Network and Transit False-positive Catalog: Pre-vetted False Positives for TESS
spellingShingle The KELT Follow-up Network and Transit False-positive Catalog: Pre-vetted False Positives for TESS
Collins, Karen A.
METHODS: OBSERVATIONAL
TECHNIQUES: PHOTOMETRIC
TECHNIQUES: RADIAL VELOCITIES
TECHNIQUES: SPECTROSCOPIC
title_short The KELT Follow-up Network and Transit False-positive Catalog: Pre-vetted False Positives for TESS
title_full The KELT Follow-up Network and Transit False-positive Catalog: Pre-vetted False Positives for TESS
title_fullStr The KELT Follow-up Network and Transit False-positive Catalog: Pre-vetted False Positives for TESS
title_full_unstemmed The KELT Follow-up Network and Transit False-positive Catalog: Pre-vetted False Positives for TESS
title_sort The KELT Follow-up Network and Transit False-positive Catalog: Pre-vetted False Positives for TESS
dc.creator.none.fl_str_mv Collins, Karen A.
Collins, Kevin I.
Pepper, Joshua
Labadie Bartz, Jonathan
Stassun, Keivan G.
Gaudi, B. Scott
Bayliss, Daniel
Bento, Joao
Colón, Knicole D.
Feliz, Dax
James, David
Johnson, Marshall C.
Kuhn, Rudolf B.
Lund, Michael B.
Penny, Matthew T.
Rodriguez, Joseph E.
Siverd, Robert J.
Stevens, Daniel J.
Yao, Xinyu
Zhou, George
Akshay, Mundra
Aldi, Giulio F.
Ashcraft, Cliff
Awiphan, Supachai
Baştürk, Özgür
Baker, David
Beatty, Thomas G.
Benni, Paul
Berlind, Perry
Berriman, Bruce G.
Petrucci, Romina Paola
Jofre, Jorge Emiliano
author Collins, Karen A.
author_facet Collins, Karen A.
Collins, Kevin I.
Pepper, Joshua
Labadie Bartz, Jonathan
Stassun, Keivan G.
Gaudi, B. Scott
Bayliss, Daniel
Bento, Joao
Colón, Knicole D.
Feliz, Dax
James, David
Johnson, Marshall C.
Kuhn, Rudolf B.
Lund, Michael B.
Penny, Matthew T.
Rodriguez, Joseph E.
Siverd, Robert J.
Stevens, Daniel J.
Yao, Xinyu
Zhou, George
Akshay, Mundra
Aldi, Giulio F.
Ashcraft, Cliff
Awiphan, Supachai
Baştürk, Özgür
Baker, David
Beatty, Thomas G.
Benni, Paul
Berlind, Perry
Berriman, Bruce G.
Petrucci, Romina Paola
Jofre, Jorge Emiliano
author_role author
author2 Collins, Kevin I.
Pepper, Joshua
Labadie Bartz, Jonathan
Stassun, Keivan G.
Gaudi, B. Scott
Bayliss, Daniel
Bento, Joao
Colón, Knicole D.
Feliz, Dax
James, David
Johnson, Marshall C.
Kuhn, Rudolf B.
Lund, Michael B.
Penny, Matthew T.
Rodriguez, Joseph E.
Siverd, Robert J.
Stevens, Daniel J.
Yao, Xinyu
Zhou, George
Akshay, Mundra
Aldi, Giulio F.
Ashcraft, Cliff
Awiphan, Supachai
Baştürk, Özgür
Baker, David
Beatty, Thomas G.
Benni, Paul
Berlind, Perry
Berriman, Bruce G.
Petrucci, Romina Paola
Jofre, Jorge Emiliano
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 METHODS: OBSERVATIONAL
TECHNIQUES: PHOTOMETRIC
TECHNIQUES: RADIAL VELOCITIES
TECHNIQUES: SPECTROSCOPIC
topic METHODS: OBSERVATIONAL
TECHNIQUES: PHOTOMETRIC
TECHNIQUES: RADIAL VELOCITIES
TECHNIQUES: SPECTROSCOPIC
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.7
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The Kilodegree Extremely Little Telescope (KELT) project has been conducting a photometric survey of transiting planets orbiting bright stars for over 10 years. The KELT images have a pixel scale of ∼23″ pixel-1 - very similar to that of NASA´s Transiting Exoplanet Survey Satellite (TESS) - as well as a large point-spread function, and the KELT reduction pipeline uses a weighted photometric aperture with radius 3′. At this angular scale, multiple stars are typically blended in the photometric apertures. In order to identify false positives and confirm transiting exoplanets, we have assembled a follow-up network (KELT-FUN) to conduct imaging with spatial resolution, cadence, and photometric precision higher than the KELT telescopes, as well as spectroscopic observations of the candidate host stars. The KELT-FUN team has followed-up over 1600 planet candidates since 2011, resulting in more than 20 planet discoveries. Excluding ∼450 false alarms of non-astrophysical origin (i.e., instrumental noise or systematics), we present an all-sky catalog of the 1128 bright stars (6 < V < 13) that show transit-like features in the KELT light curves, but which were subsequently determined to be astrophysical false positives (FPs) after photometric and/or spectroscopic follow-up observations. The KELT-FUN team continues to pursue KELT and other planet candidates and will eventually follow up certain classes of TESS candidates. The KELT FP catalog will help minimize the duplication of follow-up observations by current and future transit surveys such as TESS.
Fil: Collins, Karen A.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Collins, Kevin I.. Vanderbilt University; Estados Unidos
Fil: Pepper, Joshua. Lehigh University; Estados Unidos
Fil: Labadie Bartz, Jonathan. Lehigh University; Estados Unidos. University of Delaware; Estados Unidos
Fil: Stassun, Keivan G.. Fisk University; Estados Unidos. Vanderbilt University; Estados Unidos
Fil: Gaudi, B. Scott. Ohio State University; Estados Unidos
Fil: Bayliss, Daniel. University of Warwick; Reino Unido. Australian National University; Australia
Fil: Bento, Joao. Australian National University; Australia
Fil: Colón, Knicole D.. National Aeronautics and Space Administration; Estados Unidos. Fisk University; Estados Unidos
Fil: Feliz, Dax. Vanderbilt University; Estados Unidos
Fil: James, David. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Johnson, Marshall C.. Ohio State University; Estados Unidos
Fil: Kuhn, Rudolf B.. Southern African Large Telescope; Sudáfrica. South African Astronomical Observatory; Sudáfrica
Fil: Lund, Michael B.. Vanderbilt University; Estados Unidos
Fil: Penny, Matthew T.. Ohio State University; Estados Unidos
Fil: Rodriguez, Joseph E.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Siverd, Robert J.. Las Cumbres Observatory; Estados Unidos
Fil: Stevens, Daniel J.. Ohio State University; Estados Unidos
Fil: Yao, Xinyu. Lehigh University; Estados Unidos
Fil: Zhou, George. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. Australian National University; Australia
Fil: Akshay, Mundra. Phillips Academy; Estados Unidos
Fil: Aldi, Giulio F.. Universita di Salerno; Italia. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Ashcraft, Cliff. Union County College; Estados Unidos
Fil: Awiphan, Supachai. National Astronomical Research Institute of Thailand; Tailandia
Fil: Baştürk, Özgür. Ankara Üniversitesi. Fen Fakültesi; Turquía
Fil: Baker, David. Austin College; Estados Unidos
Fil: Beatty, Thomas G.. State University of Pennsylvania; Estados Unidos
Fil: Benni, Paul. Paul Benni Private Observatory; Estados Unidos
Fil: Berlind, Perry. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Berriman, Bruce G.. State University of Pennsylvania; Estados Unidos
Fil: Petrucci, Romina Paola. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina
Fil: Jofre, Jorge Emiliano. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba; Argentina. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina
description The Kilodegree Extremely Little Telescope (KELT) project has been conducting a photometric survey of transiting planets orbiting bright stars for over 10 years. The KELT images have a pixel scale of ∼23″ pixel-1 - very similar to that of NASA´s Transiting Exoplanet Survey Satellite (TESS) - as well as a large point-spread function, and the KELT reduction pipeline uses a weighted photometric aperture with radius 3′. At this angular scale, multiple stars are typically blended in the photometric apertures. In order to identify false positives and confirm transiting exoplanets, we have assembled a follow-up network (KELT-FUN) to conduct imaging with spatial resolution, cadence, and photometric precision higher than the KELT telescopes, as well as spectroscopic observations of the candidate host stars. The KELT-FUN team has followed-up over 1600 planet candidates since 2011, resulting in more than 20 planet discoveries. Excluding ∼450 false alarms of non-astrophysical origin (i.e., instrumental noise or systematics), we present an all-sky catalog of the 1128 bright stars (6 < V < 13) that show transit-like features in the KELT light curves, but which were subsequently determined to be astrophysical false positives (FPs) after photometric and/or spectroscopic follow-up observations. The KELT-FUN team continues to pursue KELT and other planet candidates and will eventually follow up certain classes of TESS candidates. The KELT FP catalog will help minimize the duplication of follow-up observations by current and future transit surveys such as TESS.
publishDate 2018
dc.date.none.fl_str_mv 2018-11
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/11336/164440
Collins, Karen A.; Collins, Kevin I.; Pepper, Joshua; Labadie Bartz, Jonathan; Stassun, Keivan G.; et al.; The KELT Follow-up Network and Transit False-positive Catalog: Pre-vetted False Positives for TESS; IOP Publishing; Astronomical Journal; 156; 5; 11-2018; 1-19
0004-6256
1538-3881
CONICET Digital
CONICET
url http://hdl.handle.net/11336/164440
identifier_str_mv Collins, Karen A.; Collins, Kevin I.; Pepper, Joshua; Labadie Bartz, Jonathan; Stassun, Keivan G.; et al.; The KELT Follow-up Network and Transit False-positive Catalog: Pre-vetted False Positives for TESS; IOP Publishing; Astronomical Journal; 156; 5; 11-2018; 1-19
0004-6256
1538-3881
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-3881/aae582
info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-3881/aae582
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
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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