The Calern Asteroid Polarisation Survey: An updated catalogue of asteroid polarimetric data
- Autores
- Bendjoya, P.; Cellino, A.; Rivet, J. P.; Devogèle, M.; Bagnulo, S.; Abe, L.; Vernet, D.; Gil Hutton, Ricardo Alfredo; Veneziani, A.
- Año de publicación
- 2022
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Context. The Calern Asteroid Polarimetric Survey (CAPS), a collaboration between the INAF Astrophysical Observatory of Torino (Italy) and the Observatoire de la Côte d'Azur (Nice, France), has produced new asteroid polarimetric data for a number of years, and is one of the most important, currently active projects of asteroid polarimetry. Aims. The purpose of this paper is to make public the CAPS data collected thus far, to explain the adopted techniques of data reduction and computation of phase-polarisation curves for the measured objects, and explain, by means of some examples, the importance of the CAPS database. Methods. The pipeline of data reduction has been recently updated and made as automatic as possible, using numerical algorithms developed specifically for the purposes of CAPS. The derivation of phase-polarisation curves for the observed asteroids is done using established criteria and algorithms that have recently been slightly improved, and are also summarised in this paper. Results. The CAPS catalogue is a steadily growing source of information which can be exploited for different purposes, including, but not limited to, an updated calibration of the relations existing between different polarimetric parameters and the geometric albedo of the objects, and a study of classes of objects that can be most easily identified by means of their polarimetric properties. These subjects will be more specifically discussed in separate papers. Conclusions. Asteroid polarimetry data nicely complement the results of other more commonly used techniques, including visible and IR photometry and spectroscopy. CAPS contains a lot of much-desired information about physical properties, which can hardly be inferred by means of other techniques.
Fil: Bendjoya, P.. Centre National de la Recherche Scientifique; Francia
Fil: Cellino, A.. Istituto Nazionale di Astrofisica; Italia
Fil: Rivet, J. P.. Centre National de la Recherche Scientifique; Francia
Fil: Devogèle, M.. No especifíca;
Fil: Bagnulo, S.. No especifíca;
Fil: Abe, L.. Centre National de la Recherche Scientifique; Francia
Fil: Vernet, D.. Centre National de la Recherche Scientifique; Francia
Fil: Gil Hutton, Ricardo Alfredo. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geofísica y Astronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan; Argentina
Fil: Veneziani, A.. Università di Torino; Italia - Materia
-
ASTEROIDS: GENERAL
CATALOGS
MINOR PLANETS - 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:11336/217477
Ver los metadatos del registro completo
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The Calern Asteroid Polarisation Survey: An updated catalogue of asteroid polarimetric dataBendjoya, P.Cellino, A.Rivet, J. P.Devogèle, M.Bagnulo, S.Abe, L.Vernet, D.Gil Hutton, Ricardo AlfredoVeneziani, A.ASTEROIDS: GENERALCATALOGSMINOR PLANETShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Context. The Calern Asteroid Polarimetric Survey (CAPS), a collaboration between the INAF Astrophysical Observatory of Torino (Italy) and the Observatoire de la Côte d'Azur (Nice, France), has produced new asteroid polarimetric data for a number of years, and is one of the most important, currently active projects of asteroid polarimetry. Aims. The purpose of this paper is to make public the CAPS data collected thus far, to explain the adopted techniques of data reduction and computation of phase-polarisation curves for the measured objects, and explain, by means of some examples, the importance of the CAPS database. Methods. The pipeline of data reduction has been recently updated and made as automatic as possible, using numerical algorithms developed specifically for the purposes of CAPS. The derivation of phase-polarisation curves for the observed asteroids is done using established criteria and algorithms that have recently been slightly improved, and are also summarised in this paper. Results. The CAPS catalogue is a steadily growing source of information which can be exploited for different purposes, including, but not limited to, an updated calibration of the relations existing between different polarimetric parameters and the geometric albedo of the objects, and a study of classes of objects that can be most easily identified by means of their polarimetric properties. These subjects will be more specifically discussed in separate papers. Conclusions. Asteroid polarimetry data nicely complement the results of other more commonly used techniques, including visible and IR photometry and spectroscopy. CAPS contains a lot of much-desired information about physical properties, which can hardly be inferred by means of other techniques.Fil: Bendjoya, P.. Centre National de la Recherche Scientifique; FranciaFil: Cellino, A.. Istituto Nazionale di Astrofisica; ItaliaFil: Rivet, J. P.. Centre National de la Recherche Scientifique; FranciaFil: Devogèle, M.. No especifíca;Fil: Bagnulo, S.. No especifíca;Fil: Abe, L.. Centre National de la Recherche Scientifique; FranciaFil: Vernet, D.. Centre National de la Recherche Scientifique; FranciaFil: Gil Hutton, Ricardo Alfredo. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geofísica y Astronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan; ArgentinaFil: Veneziani, A.. Università di Torino; ItaliaEDP Sciences2022-09info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/217477Bendjoya, P.; Cellino, A.; Rivet, J. P.; Devogèle, M.; Bagnulo, S.; et al.; The Calern Asteroid Polarisation Survey: An updated catalogue of asteroid polarimetric data; EDP Sciences; Astronomy and Astrophysics; 665; 9-2022; 1-170004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202142960info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:33:50Zoai:ri.conicet.gov.ar:11336/217477instacron: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 09:33:50.944CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
The Calern Asteroid Polarisation Survey: An updated catalogue of asteroid polarimetric data |
title |
The Calern Asteroid Polarisation Survey: An updated catalogue of asteroid polarimetric data |
spellingShingle |
The Calern Asteroid Polarisation Survey: An updated catalogue of asteroid polarimetric data Bendjoya, P. ASTEROIDS: GENERAL CATALOGS MINOR PLANETS |
title_short |
The Calern Asteroid Polarisation Survey: An updated catalogue of asteroid polarimetric data |
title_full |
The Calern Asteroid Polarisation Survey: An updated catalogue of asteroid polarimetric data |
title_fullStr |
The Calern Asteroid Polarisation Survey: An updated catalogue of asteroid polarimetric data |
title_full_unstemmed |
The Calern Asteroid Polarisation Survey: An updated catalogue of asteroid polarimetric data |
title_sort |
The Calern Asteroid Polarisation Survey: An updated catalogue of asteroid polarimetric data |
dc.creator.none.fl_str_mv |
Bendjoya, P. Cellino, A. Rivet, J. P. Devogèle, M. Bagnulo, S. Abe, L. Vernet, D. Gil Hutton, Ricardo Alfredo Veneziani, A. |
author |
Bendjoya, P. |
author_facet |
Bendjoya, P. Cellino, A. Rivet, J. P. Devogèle, M. Bagnulo, S. Abe, L. Vernet, D. Gil Hutton, Ricardo Alfredo Veneziani, A. |
author_role |
author |
author2 |
Cellino, A. Rivet, J. P. Devogèle, M. Bagnulo, S. Abe, L. Vernet, D. Gil Hutton, Ricardo Alfredo Veneziani, A. |
author2_role |
author author author author author author author author |
dc.subject.none.fl_str_mv |
ASTEROIDS: GENERAL CATALOGS MINOR PLANETS |
topic |
ASTEROIDS: GENERAL CATALOGS MINOR PLANETS |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Context. The Calern Asteroid Polarimetric Survey (CAPS), a collaboration between the INAF Astrophysical Observatory of Torino (Italy) and the Observatoire de la Côte d'Azur (Nice, France), has produced new asteroid polarimetric data for a number of years, and is one of the most important, currently active projects of asteroid polarimetry. Aims. The purpose of this paper is to make public the CAPS data collected thus far, to explain the adopted techniques of data reduction and computation of phase-polarisation curves for the measured objects, and explain, by means of some examples, the importance of the CAPS database. Methods. The pipeline of data reduction has been recently updated and made as automatic as possible, using numerical algorithms developed specifically for the purposes of CAPS. The derivation of phase-polarisation curves for the observed asteroids is done using established criteria and algorithms that have recently been slightly improved, and are also summarised in this paper. Results. The CAPS catalogue is a steadily growing source of information which can be exploited for different purposes, including, but not limited to, an updated calibration of the relations existing between different polarimetric parameters and the geometric albedo of the objects, and a study of classes of objects that can be most easily identified by means of their polarimetric properties. These subjects will be more specifically discussed in separate papers. Conclusions. Asteroid polarimetry data nicely complement the results of other more commonly used techniques, including visible and IR photometry and spectroscopy. CAPS contains a lot of much-desired information about physical properties, which can hardly be inferred by means of other techniques. Fil: Bendjoya, P.. Centre National de la Recherche Scientifique; Francia Fil: Cellino, A.. Istituto Nazionale di Astrofisica; Italia Fil: Rivet, J. P.. Centre National de la Recherche Scientifique; Francia Fil: Devogèle, M.. No especifíca; Fil: Bagnulo, S.. No especifíca; Fil: Abe, L.. Centre National de la Recherche Scientifique; Francia Fil: Vernet, D.. Centre National de la Recherche Scientifique; Francia Fil: Gil Hutton, Ricardo Alfredo. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geofísica y Astronomía; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan; Argentina Fil: Veneziani, A.. Università di Torino; Italia |
description |
Context. The Calern Asteroid Polarimetric Survey (CAPS), a collaboration between the INAF Astrophysical Observatory of Torino (Italy) and the Observatoire de la Côte d'Azur (Nice, France), has produced new asteroid polarimetric data for a number of years, and is one of the most important, currently active projects of asteroid polarimetry. Aims. The purpose of this paper is to make public the CAPS data collected thus far, to explain the adopted techniques of data reduction and computation of phase-polarisation curves for the measured objects, and explain, by means of some examples, the importance of the CAPS database. Methods. The pipeline of data reduction has been recently updated and made as automatic as possible, using numerical algorithms developed specifically for the purposes of CAPS. The derivation of phase-polarisation curves for the observed asteroids is done using established criteria and algorithms that have recently been slightly improved, and are also summarised in this paper. Results. The CAPS catalogue is a steadily growing source of information which can be exploited for different purposes, including, but not limited to, an updated calibration of the relations existing between different polarimetric parameters and the geometric albedo of the objects, and a study of classes of objects that can be most easily identified by means of their polarimetric properties. These subjects will be more specifically discussed in separate papers. Conclusions. Asteroid polarimetry data nicely complement the results of other more commonly used techniques, including visible and IR photometry and spectroscopy. CAPS contains a lot of much-desired information about physical properties, which can hardly be inferred by means of other techniques. |
publishDate |
2022 |
dc.date.none.fl_str_mv |
2022-09 |
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/11336/217477 Bendjoya, P.; Cellino, A.; Rivet, J. P.; Devogèle, M.; Bagnulo, S.; et al.; The Calern Asteroid Polarisation Survey: An updated catalogue of asteroid polarimetric data; EDP Sciences; Astronomy and Astrophysics; 665; 9-2022; 1-17 0004-6361 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/217477 |
identifier_str_mv |
Bendjoya, P.; Cellino, A.; Rivet, J. P.; Devogèle, M.; Bagnulo, S.; et al.; The Calern Asteroid Polarisation Survey: An updated catalogue of asteroid polarimetric data; EDP Sciences; Astronomy and Astrophysics; 665; 9-2022; 1-17 0004-6361 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202142960 |
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 |
EDP Sciences |
publisher.none.fl_str_mv |
EDP Sciences |
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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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 |