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
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/164440
Ver los metadatos del registro completo
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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 Técnicas2025-10-22T11:38:57Zoai: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:34982025-10-22 11:38:57.704CONICET 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 |
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info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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openAccess |
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https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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IOP Publishing |
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IOP Publishing |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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