Enhancing Exoplanet Ephemerides by Leveraging Professional and Citizen Science Data: A Test Case with WASP-77 A b
- Autores
- Noguer, Federico R.; Corley, Suber; Pearson, Kyle A.; Zellem, Robert T.; Simon, Molly N.; Burt, Jennifer A.; Huckabee, Isabela; August, Prune C.; Weiner Mansfield, Megan; Dalba, Paul A.; Smith, Peter C. B.; Banks, Timothy; Bell, Ira; Daniel, Dominique; Dawson, Lindsay; De Mula, Jesús; Deldem, Marc; Deligeorgopoulos, Dimitrios; Di Sisto, Romina Paula; Dymock, Roger; Evans, Phil; Follero, Giulio; Fowler, Martin J. F.; Fernandez Lajus, Eduardo Eusebio; Hamrick, Alex; Iannascoli, Nicoletta; Kovacs, Andre O.; Kulh, Denis Henrique; Lopresti, Claudio; Marino, Antonio
- Año de publicación
- 2024
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present an updated ephemeris, and physical parameters, for the exoplanet WASP-77 A b. In this effort, we combine 64 ground- and space-based transit observations, 6 space-based eclipse observations, and 32 radial velocity observations to produce this target´s most precise orbital solution to date aiding in the planning of James Webb Space Telescope and Ariel observations and atmospheric studies. We report a new orbital period of 1.360029395 ± 5.7 × 10−8 days, a new mid-transit time of 2459957.337860 ± 4.3 × 10−5 Barycentric Julian Date in the Barycentric Dynamical Timescale (BJDTDB) and a new mid-eclipse time of 2459956.658192 ± 6.7 × 10−5 BJDTDB. Furthermore, the methods presented in this study reduce the uncertainties in the planet´s mass 1.6654 ± 4.5 × 10−3MJup and orbital period 1.360029395 ± 5.7 × 10−8 days by factors of 15.1 and 10.9, respectively. Through a joint fit analysis comparison of transit data taken by space-based and citizen science-led initiatives, our study demonstrates the power of including data collected by citizen scientists compared to a fit of the space-based data alone. Additionally, by including a vast array of citizen science data from ExoClock, Exoplanet Transit Database, and Exoplanet Watch, we can increase our observational baseline and thus acquire better constraints on the forward propagation of our ephemeris than what is achievable with Transiting Exoplanet Survey Satellite data alone.
Fil: Noguer, Federico R.. Arizona State University; Estados Unidos
Fil: Corley, Suber. National Aeronautics and Space Administration; Estados Unidos
Fil: Pearson, Kyle A.. California Institute Of Technology; Estados Unidos
Fil: Zellem, Robert T.. California Institute Of Technology; Estados Unidos
Fil: Simon, Molly N.. Arizona State University; Estados Unidos
Fil: Burt, Jennifer A.. California Institute Of Technology; Estados Unidos
Fil: Huckabee, Isabela. California Institute Of Technology; Estados Unidos
Fil: August, Prune C.. Technical University of Denmark; Dinamarca
Fil: Weiner Mansfield, Megan. University of Arizona; Estados Unidos
Fil: Dalba, Paul A.. University of California; Estados Unidos
Fil: Smith, Peter C. B.. Arizona State University; Estados Unidos
Fil: Banks, Timothy. Harper College; Estados Unidos
Fil: Bell, Ira. Arizona State University; Estados Unidos
Fil: Daniel, Dominique. ExoClock Project Citizen Scientist; Estados Unidos
Fil: Dawson, Lindsay. Thomas More University; Estados Unidos
Fil: De Mula, Jesús. Exoplanet Watch Citizen Scientist Contributor; Estados Unidos
Fil: Deldem, Marc. ExoClock Project Citizen Scientist Contributor; Estados Unidos
Fil: Deligeorgopoulos, Dimitrios. ExoClock Project Citizen Scientist Contributor; Estados Unidos
Fil: Di Sisto, Romina Paula. 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: Dymock, Roger. British Astronomical Association; Reino Unido
Fil: Evans, Phil. El Sauce Observatory; Chile
Fil: Follero, Giulio. INAF. Osservatorio Astronomico di Capodimonte; Italia
Fil: Fowler, Martin J. F.. Les Rocquettes Observatory and Exoplanet Factory; Reino Unido
Fil: Fernandez Lajus, Eduardo Eusebio. 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: Hamrick, Alex. Stanford Online High School; Estados Unidos
Fil: Iannascoli, Nicoletta. INAF. Osservatorio Astronomico di Capodimonte; Italia
Fil: Kovacs, Andre O.. Exoplanet Watch Citizen Scientist Contributor; Estados Unidos
Fil: Kulh, Denis Henrique. Alfa Crucis; Estados Unidos
Fil: Lopresti, Claudio. ExoClock Project Citizen Scientist Contributor; Estados Unidos
Fil: Marino, Antonio. INAF. Osservatorio Astronomico di Capodimonte; Italia - Materia
- exoplanets
- Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/245277
Ver los metadatos del registro completo
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Enhancing Exoplanet Ephemerides by Leveraging Professional and Citizen Science Data: A Test Case with WASP-77 A bNoguer, Federico R.Corley, SuberPearson, Kyle A.Zellem, Robert T.Simon, Molly N.Burt, Jennifer A.Huckabee, IsabelaAugust, Prune C.Weiner Mansfield, MeganDalba, Paul A.Smith, Peter C. B.Banks, TimothyBell, IraDaniel, DominiqueDawson, LindsayDe Mula, JesúsDeldem, MarcDeligeorgopoulos, DimitriosDi Sisto, Romina PaulaDymock, RogerEvans, PhilFollero, GiulioFowler, Martin J. F.Fernandez Lajus, Eduardo EusebioHamrick, AlexIannascoli, NicolettaKovacs, Andre O.Kulh, Denis HenriqueLopresti, ClaudioMarino, Antonioexoplanetshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present an updated ephemeris, and physical parameters, for the exoplanet WASP-77 A b. In this effort, we combine 64 ground- and space-based transit observations, 6 space-based eclipse observations, and 32 radial velocity observations to produce this target´s most precise orbital solution to date aiding in the planning of James Webb Space Telescope and Ariel observations and atmospheric studies. We report a new orbital period of 1.360029395 ± 5.7 × 10−8 days, a new mid-transit time of 2459957.337860 ± 4.3 × 10−5 Barycentric Julian Date in the Barycentric Dynamical Timescale (BJDTDB) and a new mid-eclipse time of 2459956.658192 ± 6.7 × 10−5 BJDTDB. Furthermore, the methods presented in this study reduce the uncertainties in the planet´s mass 1.6654 ± 4.5 × 10−3MJup and orbital period 1.360029395 ± 5.7 × 10−8 days by factors of 15.1 and 10.9, respectively. Through a joint fit analysis comparison of transit data taken by space-based and citizen science-led initiatives, our study demonstrates the power of including data collected by citizen scientists compared to a fit of the space-based data alone. Additionally, by including a vast array of citizen science data from ExoClock, Exoplanet Transit Database, and Exoplanet Watch, we can increase our observational baseline and thus acquire better constraints on the forward propagation of our ephemeris than what is achievable with Transiting Exoplanet Survey Satellite data alone.Fil: Noguer, Federico R.. Arizona State University; Estados UnidosFil: Corley, Suber. National Aeronautics and Space Administration; Estados UnidosFil: Pearson, Kyle A.. California Institute Of Technology; Estados UnidosFil: Zellem, Robert T.. California Institute Of Technology; Estados UnidosFil: Simon, Molly N.. Arizona State University; Estados UnidosFil: Burt, Jennifer A.. California Institute Of Technology; Estados UnidosFil: Huckabee, Isabela. California Institute Of Technology; Estados UnidosFil: August, Prune C.. Technical University of Denmark; DinamarcaFil: Weiner Mansfield, Megan. University of Arizona; Estados UnidosFil: Dalba, Paul A.. University of California; Estados UnidosFil: Smith, Peter C. B.. Arizona State University; Estados UnidosFil: Banks, Timothy. Harper College; Estados UnidosFil: Bell, Ira. Arizona State University; Estados UnidosFil: Daniel, Dominique. ExoClock Project Citizen Scientist; Estados UnidosFil: Dawson, Lindsay. Thomas More University; Estados UnidosFil: De Mula, Jesús. Exoplanet Watch Citizen Scientist Contributor; Estados UnidosFil: Deldem, Marc. ExoClock Project Citizen Scientist Contributor; Estados UnidosFil: Deligeorgopoulos, Dimitrios. ExoClock Project Citizen Scientist Contributor; Estados UnidosFil: Di Sisto, Romina Paula. 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: Dymock, Roger. British Astronomical Association; Reino UnidoFil: Evans, Phil. El Sauce Observatory; ChileFil: Follero, Giulio. INAF. Osservatorio Astronomico di Capodimonte; ItaliaFil: Fowler, Martin J. F.. Les Rocquettes Observatory and Exoplanet Factory; Reino UnidoFil: Fernandez Lajus, Eduardo Eusebio. 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: Hamrick, Alex. Stanford Online High School; Estados UnidosFil: Iannascoli, Nicoletta. INAF. Osservatorio Astronomico di Capodimonte; ItaliaFil: Kovacs, Andre O.. Exoplanet Watch Citizen Scientist Contributor; Estados UnidosFil: Kulh, Denis Henrique. Alfa Crucis; Estados UnidosFil: Lopresti, Claudio. ExoClock Project Citizen Scientist Contributor; Estados UnidosFil: Marino, Antonio. INAF. Osservatorio Astronomico di Capodimonte; ItaliaIOP 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/11336/245277Noguer, Federico R.; Corley, Suber; Pearson, Kyle A.; Zellem, Robert T.; Simon, Molly N.; et al.; Enhancing Exoplanet Ephemerides by Leveraging Professional and Citizen Science Data: A Test Case with WASP-77 A b; IOP Publishing; Publications of the Astronomical Society of the Pacific; 136; 6; 7-2024; 1-280004-6280CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/1538-3873/ad57f5info:eu-repo/semantics/altIdentifier/doi/10.1088/1538-3873/ad57f5info:eu-repo/semantics/altIdentifier/url/.info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:40:09Zoai:ri.conicet.gov.ar:11336/245277instacron: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 09:40:09.654CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Enhancing Exoplanet Ephemerides by Leveraging Professional and Citizen Science Data: A Test Case with WASP-77 A b |
title |
Enhancing Exoplanet Ephemerides by Leveraging Professional and Citizen Science Data: A Test Case with WASP-77 A b |
spellingShingle |
Enhancing Exoplanet Ephemerides by Leveraging Professional and Citizen Science Data: A Test Case with WASP-77 A b Noguer, Federico R. exoplanets |
title_short |
Enhancing Exoplanet Ephemerides by Leveraging Professional and Citizen Science Data: A Test Case with WASP-77 A b |
title_full |
Enhancing Exoplanet Ephemerides by Leveraging Professional and Citizen Science Data: A Test Case with WASP-77 A b |
title_fullStr |
Enhancing Exoplanet Ephemerides by Leveraging Professional and Citizen Science Data: A Test Case with WASP-77 A b |
title_full_unstemmed |
Enhancing Exoplanet Ephemerides by Leveraging Professional and Citizen Science Data: A Test Case with WASP-77 A b |
title_sort |
Enhancing Exoplanet Ephemerides by Leveraging Professional and Citizen Science Data: A Test Case with WASP-77 A b |
dc.creator.none.fl_str_mv |
Noguer, Federico R. Corley, Suber Pearson, Kyle A. Zellem, Robert T. Simon, Molly N. Burt, Jennifer A. Huckabee, Isabela August, Prune C. Weiner Mansfield, Megan Dalba, Paul A. Smith, Peter C. B. Banks, Timothy Bell, Ira Daniel, Dominique Dawson, Lindsay De Mula, Jesús Deldem, Marc Deligeorgopoulos, Dimitrios Di Sisto, Romina Paula Dymock, Roger Evans, Phil Follero, Giulio Fowler, Martin J. F. Fernandez Lajus, Eduardo Eusebio Hamrick, Alex Iannascoli, Nicoletta Kovacs, Andre O. Kulh, Denis Henrique Lopresti, Claudio Marino, Antonio |
author |
Noguer, Federico R. |
author_facet |
Noguer, Federico R. Corley, Suber Pearson, Kyle A. Zellem, Robert T. Simon, Molly N. Burt, Jennifer A. Huckabee, Isabela August, Prune C. Weiner Mansfield, Megan Dalba, Paul A. Smith, Peter C. B. Banks, Timothy Bell, Ira Daniel, Dominique Dawson, Lindsay De Mula, Jesús Deldem, Marc Deligeorgopoulos, Dimitrios Di Sisto, Romina Paula Dymock, Roger Evans, Phil Follero, Giulio Fowler, Martin J. F. Fernandez Lajus, Eduardo Eusebio Hamrick, Alex Iannascoli, Nicoletta Kovacs, Andre O. Kulh, Denis Henrique Lopresti, Claudio Marino, Antonio |
author_role |
author |
author2 |
Corley, Suber Pearson, Kyle A. Zellem, Robert T. Simon, Molly N. Burt, Jennifer A. Huckabee, Isabela August, Prune C. Weiner Mansfield, Megan Dalba, Paul A. Smith, Peter C. B. Banks, Timothy Bell, Ira Daniel, Dominique Dawson, Lindsay De Mula, Jesús Deldem, Marc Deligeorgopoulos, Dimitrios Di Sisto, Romina Paula Dymock, Roger Evans, Phil Follero, Giulio Fowler, Martin J. F. Fernandez Lajus, Eduardo Eusebio Hamrick, Alex Iannascoli, Nicoletta Kovacs, Andre O. Kulh, Denis Henrique Lopresti, Claudio Marino, Antonio |
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 |
exoplanets |
topic |
exoplanets |
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 updated ephemeris, and physical parameters, for the exoplanet WASP-77 A b. In this effort, we combine 64 ground- and space-based transit observations, 6 space-based eclipse observations, and 32 radial velocity observations to produce this target´s most precise orbital solution to date aiding in the planning of James Webb Space Telescope and Ariel observations and atmospheric studies. We report a new orbital period of 1.360029395 ± 5.7 × 10−8 days, a new mid-transit time of 2459957.337860 ± 4.3 × 10−5 Barycentric Julian Date in the Barycentric Dynamical Timescale (BJDTDB) and a new mid-eclipse time of 2459956.658192 ± 6.7 × 10−5 BJDTDB. Furthermore, the methods presented in this study reduce the uncertainties in the planet´s mass 1.6654 ± 4.5 × 10−3MJup and orbital period 1.360029395 ± 5.7 × 10−8 days by factors of 15.1 and 10.9, respectively. Through a joint fit analysis comparison of transit data taken by space-based and citizen science-led initiatives, our study demonstrates the power of including data collected by citizen scientists compared to a fit of the space-based data alone. Additionally, by including a vast array of citizen science data from ExoClock, Exoplanet Transit Database, and Exoplanet Watch, we can increase our observational baseline and thus acquire better constraints on the forward propagation of our ephemeris than what is achievable with Transiting Exoplanet Survey Satellite data alone. Fil: Noguer, Federico R.. Arizona State University; Estados Unidos Fil: Corley, Suber. National Aeronautics and Space Administration; Estados Unidos Fil: Pearson, Kyle A.. California Institute Of Technology; Estados Unidos Fil: Zellem, Robert T.. California Institute Of Technology; Estados Unidos Fil: Simon, Molly N.. Arizona State University; Estados Unidos Fil: Burt, Jennifer A.. California Institute Of Technology; Estados Unidos Fil: Huckabee, Isabela. California Institute Of Technology; Estados Unidos Fil: August, Prune C.. Technical University of Denmark; Dinamarca Fil: Weiner Mansfield, Megan. University of Arizona; Estados Unidos Fil: Dalba, Paul A.. University of California; Estados Unidos Fil: Smith, Peter C. B.. Arizona State University; Estados Unidos Fil: Banks, Timothy. Harper College; Estados Unidos Fil: Bell, Ira. Arizona State University; Estados Unidos Fil: Daniel, Dominique. ExoClock Project Citizen Scientist; Estados Unidos Fil: Dawson, Lindsay. Thomas More University; Estados Unidos Fil: De Mula, Jesús. Exoplanet Watch Citizen Scientist Contributor; Estados Unidos Fil: Deldem, Marc. ExoClock Project Citizen Scientist Contributor; Estados Unidos Fil: Deligeorgopoulos, Dimitrios. ExoClock Project Citizen Scientist Contributor; Estados Unidos Fil: Di Sisto, Romina Paula. 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: Dymock, Roger. British Astronomical Association; Reino Unido Fil: Evans, Phil. El Sauce Observatory; Chile Fil: Follero, Giulio. INAF. Osservatorio Astronomico di Capodimonte; Italia Fil: Fowler, Martin J. F.. Les Rocquettes Observatory and Exoplanet Factory; Reino Unido Fil: Fernandez Lajus, Eduardo Eusebio. 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: Hamrick, Alex. Stanford Online High School; Estados Unidos Fil: Iannascoli, Nicoletta. INAF. Osservatorio Astronomico di Capodimonte; Italia Fil: Kovacs, Andre O.. Exoplanet Watch Citizen Scientist Contributor; Estados Unidos Fil: Kulh, Denis Henrique. Alfa Crucis; Estados Unidos Fil: Lopresti, Claudio. ExoClock Project Citizen Scientist Contributor; Estados Unidos Fil: Marino, Antonio. INAF. Osservatorio Astronomico di Capodimonte; Italia |
description |
We present an updated ephemeris, and physical parameters, for the exoplanet WASP-77 A b. In this effort, we combine 64 ground- and space-based transit observations, 6 space-based eclipse observations, and 32 radial velocity observations to produce this target´s most precise orbital solution to date aiding in the planning of James Webb Space Telescope and Ariel observations and atmospheric studies. We report a new orbital period of 1.360029395 ± 5.7 × 10−8 days, a new mid-transit time of 2459957.337860 ± 4.3 × 10−5 Barycentric Julian Date in the Barycentric Dynamical Timescale (BJDTDB) and a new mid-eclipse time of 2459956.658192 ± 6.7 × 10−5 BJDTDB. Furthermore, the methods presented in this study reduce the uncertainties in the planet´s mass 1.6654 ± 4.5 × 10−3MJup and orbital period 1.360029395 ± 5.7 × 10−8 days by factors of 15.1 and 10.9, respectively. Through a joint fit analysis comparison of transit data taken by space-based and citizen science-led initiatives, our study demonstrates the power of including data collected by citizen scientists compared to a fit of the space-based data alone. Additionally, by including a vast array of citizen science data from ExoClock, Exoplanet Transit Database, and Exoplanet Watch, we can increase our observational baseline and thus acquire better constraints on the forward propagation of our ephemeris than what is achievable with Transiting Exoplanet Survey Satellite data alone. |
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/11336/245277 Noguer, Federico R.; Corley, Suber; Pearson, Kyle A.; Zellem, Robert T.; Simon, Molly N.; et al.; Enhancing Exoplanet Ephemerides by Leveraging Professional and Citizen Science Data: A Test Case with WASP-77 A b; IOP Publishing; Publications of the Astronomical Society of the Pacific; 136; 6; 7-2024; 1-28 0004-6280 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/245277 |
identifier_str_mv |
Noguer, Federico R.; Corley, Suber; Pearson, Kyle A.; Zellem, Robert T.; Simon, Molly N.; et al.; Enhancing Exoplanet Ephemerides by Leveraging Professional and Citizen Science Data: A Test Case with WASP-77 A b; IOP Publishing; Publications of the Astronomical Society of the Pacific; 136; 6; 7-2024; 1-28 0004-6280 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/10.1088/1538-3873/ad57f5 info:eu-repo/semantics/altIdentifier/doi/10.1088/1538-3873/ad57f5 info:eu-repo/semantics/altIdentifier/url/. |
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 |
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CONICET Digital (CONICET) |
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CONICET Digital (CONICET) |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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13.070432 |