Easy asteroid phase curve fitting for the Python ecosystem: Pyedra
- Autores
- Colazo, Milagros Rita; Cabral, Juan Bautista; Chalela Garcia, Martin; Sánchez, Bruno Orlando
- Año de publicación
- 2022
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- A trending astronomical phenomenon is the variation in brightness of asteroids. This can be caused by its rotation on its own axis and/or its position relative to the sun. The latter behavior can be visualized on a phase curve, which shows the reduced magnitude as a function of the phase angle. To enable the comparison between several models for the dependence of reduced magnitude on phase angle we present a Python package called Pyedra. Pyedra implements three phase-curve-models, and also provides tools for visualization as well as integration with external datasets. The package is fully documented and tested following a strict quality-assurance workflow, with a user-friendly programmatic interface. In future versions, we will include more models, and additional estimation of quantities derived from parameters such as diameter and different albedos, and correlation of information of physical and orbital parameters.
Fil: Colazo, Milagros Rita. Universidad Nacional de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Cabral, Juan Bautista. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Centro de Investigaciones en Química Biológica de Córdoba. Universidad Nacional de Córdoba. Facultad de Ciencias Químicas. Centro de Investigaciones en Química Biológica de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Chalela Garcia, Martin. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Sánchez, Bruno Orlando. University of Duke; Estados Unidos - Materia
-
ASTEROIDS
FUNDAMENTAL PARAMETERS
GENERAL
MINOR PLANETS
PLANETS AND SATELLITES
PYTHON PACKAGE - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-nd/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/202765
Ver los metadatos del registro completo
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oai:ri.conicet.gov.ar:11336/202765 |
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Easy asteroid phase curve fitting for the Python ecosystem: PyedraColazo, Milagros RitaCabral, Juan BautistaChalela Garcia, MartinSánchez, Bruno OrlandoASTEROIDSFUNDAMENTAL PARAMETERSGENERALMINOR PLANETSPLANETS AND SATELLITESPYTHON PACKAGEhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1https://purl.org/becyt/ford/1.2https://purl.org/becyt/ford/1A trending astronomical phenomenon is the variation in brightness of asteroids. This can be caused by its rotation on its own axis and/or its position relative to the sun. The latter behavior can be visualized on a phase curve, which shows the reduced magnitude as a function of the phase angle. To enable the comparison between several models for the dependence of reduced magnitude on phase angle we present a Python package called Pyedra. Pyedra implements three phase-curve-models, and also provides tools for visualization as well as integration with external datasets. The package is fully documented and tested following a strict quality-assurance workflow, with a user-friendly programmatic interface. In future versions, we will include more models, and additional estimation of quantities derived from parameters such as diameter and different albedos, and correlation of information of physical and orbital parameters.Fil: Colazo, Milagros Rita. Universidad Nacional de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Cabral, Juan Bautista. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Centro de Investigaciones en Química Biológica de Córdoba. Universidad Nacional de Córdoba. Facultad de Ciencias Químicas. Centro de Investigaciones en Química Biológica de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Chalela Garcia, Martin. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Sánchez, Bruno Orlando. University of Duke; Estados UnidosElsevier B.V.2022-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/202765Colazo, Milagros Rita; Cabral, Juan Bautista; Chalela Garcia, Martin; Sánchez, Bruno Orlando; Easy asteroid phase curve fitting for the Python ecosystem: Pyedra; Elsevier B.V.; Astronomy and Computing; 38; 100533; 1-2022; 1-52213-1337CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1016/j.ascom.2021.100533info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S2213133721000809info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/2103.06856info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-nd/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:41:46Zoai:ri.conicet.gov.ar:11336/202765instacron: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 09:41:46.557CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Easy asteroid phase curve fitting for the Python ecosystem: Pyedra |
title |
Easy asteroid phase curve fitting for the Python ecosystem: Pyedra |
spellingShingle |
Easy asteroid phase curve fitting for the Python ecosystem: Pyedra Colazo, Milagros Rita ASTEROIDS FUNDAMENTAL PARAMETERS GENERAL MINOR PLANETS PLANETS AND SATELLITES PYTHON PACKAGE |
title_short |
Easy asteroid phase curve fitting for the Python ecosystem: Pyedra |
title_full |
Easy asteroid phase curve fitting for the Python ecosystem: Pyedra |
title_fullStr |
Easy asteroid phase curve fitting for the Python ecosystem: Pyedra |
title_full_unstemmed |
Easy asteroid phase curve fitting for the Python ecosystem: Pyedra |
title_sort |
Easy asteroid phase curve fitting for the Python ecosystem: Pyedra |
dc.creator.none.fl_str_mv |
Colazo, Milagros Rita Cabral, Juan Bautista Chalela Garcia, Martin Sánchez, Bruno Orlando |
author |
Colazo, Milagros Rita |
author_facet |
Colazo, Milagros Rita Cabral, Juan Bautista Chalela Garcia, Martin Sánchez, Bruno Orlando |
author_role |
author |
author2 |
Cabral, Juan Bautista Chalela Garcia, Martin Sánchez, Bruno Orlando |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
ASTEROIDS FUNDAMENTAL PARAMETERS GENERAL MINOR PLANETS PLANETS AND SATELLITES PYTHON PACKAGE |
topic |
ASTEROIDS FUNDAMENTAL PARAMETERS GENERAL MINOR PLANETS PLANETS AND SATELLITES PYTHON PACKAGE |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 https://purl.org/becyt/ford/1.2 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
A trending astronomical phenomenon is the variation in brightness of asteroids. This can be caused by its rotation on its own axis and/or its position relative to the sun. The latter behavior can be visualized on a phase curve, which shows the reduced magnitude as a function of the phase angle. To enable the comparison between several models for the dependence of reduced magnitude on phase angle we present a Python package called Pyedra. Pyedra implements three phase-curve-models, and also provides tools for visualization as well as integration with external datasets. The package is fully documented and tested following a strict quality-assurance workflow, with a user-friendly programmatic interface. In future versions, we will include more models, and additional estimation of quantities derived from parameters such as diameter and different albedos, and correlation of information of physical and orbital parameters. Fil: Colazo, Milagros Rita. Universidad Nacional de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina Fil: Cabral, Juan Bautista. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Centro de Investigaciones en Química Biológica de Córdoba. Universidad Nacional de Córdoba. Facultad de Ciencias Químicas. Centro de Investigaciones en Química Biológica de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Chalela Garcia, Martin. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina Fil: Sánchez, Bruno Orlando. University of Duke; Estados Unidos |
description |
A trending astronomical phenomenon is the variation in brightness of asteroids. This can be caused by its rotation on its own axis and/or its position relative to the sun. The latter behavior can be visualized on a phase curve, which shows the reduced magnitude as a function of the phase angle. To enable the comparison between several models for the dependence of reduced magnitude on phase angle we present a Python package called Pyedra. Pyedra implements three phase-curve-models, and also provides tools for visualization as well as integration with external datasets. The package is fully documented and tested following a strict quality-assurance workflow, with a user-friendly programmatic interface. In future versions, we will include more models, and additional estimation of quantities derived from parameters such as diameter and different albedos, and correlation of information of physical and orbital parameters. |
publishDate |
2022 |
dc.date.none.fl_str_mv |
2022-01 |
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/11336/202765 Colazo, Milagros Rita; Cabral, Juan Bautista; Chalela Garcia, Martin; Sánchez, Bruno Orlando; Easy asteroid phase curve fitting for the Python ecosystem: Pyedra; Elsevier B.V.; Astronomy and Computing; 38; 100533; 1-2022; 1-5 2213-1337 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/202765 |
identifier_str_mv |
Colazo, Milagros Rita; Cabral, Juan Bautista; Chalela Garcia, Martin; Sánchez, Bruno Orlando; Easy asteroid phase curve fitting for the Python ecosystem: Pyedra; Elsevier B.V.; Astronomy and Computing; 38; 100533; 1-2022; 1-5 2213-1337 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1016/j.ascom.2021.100533 info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S2213133721000809 info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/2103.06856 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-nd/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-nd/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Elsevier B.V. |
publisher.none.fl_str_mv |
Elsevier B.V. |
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) |
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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13.070432 |