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dc.contributor.author
Bendjoya, P.  
dc.contributor.author
Cellino, A.  
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Rivet, J. P.  
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Devogèle, M.  
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Bagnulo, S.  
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Abe, L.  
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Vernet, D.  
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Gil Hutton, Ricardo Alfredo  
dc.contributor.author
Veneziani, A.  
dc.date.available
2023-11-08T15:24:05Z  
dc.date.issued
2022-09  
dc.identifier.citation
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  
dc.identifier.issn
0004-6361  
dc.identifier.uri
http://hdl.handle.net/11336/217477  
dc.description.abstract
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.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
EDP Sciences  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
ASTEROIDS: GENERAL  
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CATALOGS  
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MINOR PLANETS  
dc.subject.classification
Astronomía  
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Ciencias Físicas  
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CIENCIAS NATURALES Y EXACTAS  
dc.title
The Calern Asteroid Polarisation Survey: An updated catalogue of asteroid polarimetric data  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2023-11-07T14:28:50Z  
dc.journal.volume
665  
dc.journal.pagination
1-17  
dc.journal.pais
Francia  
dc.description.fil
Fil: Bendjoya, P.. Centre National de la Recherche Scientifique; Francia  
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Fil: Cellino, A.. Istituto Nazionale di Astrofisica; Italia  
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Fil: Rivet, J. P.. Centre National de la Recherche Scientifique; Francia  
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Fil: Devogèle, M.. No especifíca;  
dc.description.fil
Fil: Bagnulo, S.. No especifíca;  
dc.description.fil
Fil: Abe, L.. Centre National de la Recherche Scientifique; Francia  
dc.description.fil
Fil: Vernet, D.. Centre National de la Recherche Scientifique; Francia  
dc.description.fil
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  
dc.description.fil
Fil: Veneziani, A.. Università di Torino; Italia  
dc.journal.title
Astronomy and Astrophysics  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1051/0004-6361/202142960