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dc.contributor.author
Cellino, A.
dc.contributor.author
Bagnulo, S.
dc.contributor.author
Gil Hutton, Ricardo Alfredo
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Tanga, P.
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Cañada Assandri, Marcela Inés
dc.contributor.author
Tedesco, E.
dc.date.available
2016-03-23T12:26:38Z
dc.date.issued
2015-08
dc.identifier.citation
Cellino, A.; Bagnulo, S.; Gil Hutton, Ricardo Alfredo; Tanga, P.; Cañada Assandri, Marcela Inés; et al.; On the calibration of the relation between geometric albedo and polarimetric properties for the asteroids; Oxford University Press; Monthly Notices Of The Royal Astronomical Society; 451; 4; 8-2015; 3473-3488
dc.identifier.issn
0035-8711
dc.identifier.uri
http://hdl.handle.net/11336/4911
dc.description.abstract
We present a new extensive analysis of the old problem of finding a satisfactory calibration of the relation between the geometric albedo and some measurable polarization properties of the asteroids. To achieve our goals, we use all polarimetric data at our disposal. For the purposes of calibration, we use a limited sample of objects for which we can be confident to know the albedo with good accuracy, according to previous investigations of other authors. We find a new set of updated calibration coefficients for the classical slope–albedo relation, but we generalize our analysis and we consider also alternative possibilities, including the use of other polarimetric parameters, one being proposed here for the first time, and the possibility to exclude from best-fitting analyses the asteroids having low albedos. We also consider a possible parabolic fit of the whole set of data.
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
Oxford University Press
dc.rights
info:eu-repo/semantics/openAccess
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject
Techniques: Polarimetric
dc.subject
Minor Planets
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Asteroids: General
dc.subject.classification
Astronomía
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Ciencias Físicas
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CIENCIAS NATURALES Y EXACTAS
dc.title
On the calibration of the relation between geometric albedo and polarimetric properties for the asteroids
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2016-03-30 10:35:44.97925-03
dc.journal.volume
451
dc.journal.number
4
dc.journal.pagination
3473-3488
dc.journal.pais
Reino Unido
dc.journal.ciudad
Oxford
dc.conicet.avisoEditorial
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2015 The Authors] Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
dc.description.fil
Fil: Cellino, A.. Osservatorio Astrofisico di Torino; Italia
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Fil: Bagnulo, S.. Armagh Observatory; Reino Unido
dc.description.fil
Fil: Gil Hutton, Ricardo Alfredo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico San Juan. Complejo Astronómico "El Leoncito"; Argentina. Universidad Nacional de San Juan; Argentina
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Fil: Tanga, P.. Observatoire de la Cote d’Azur; Francia
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Fil: Cañada Assandri, Marcela Inés. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico San Juan. Complejo Astronómico "El Leoncito"; Argentina. Universidad Nacional de San Juan; Argentina
dc.description.fil
Fil: Tedesco, E.. Universidad Nacional de San Juan. Facultad de Ciencias Exactas, Físicas y Naturales. Departamento de Geofísica y Astronomía; Argentina
dc.journal.title
Monthly Notices Of The Royal Astronomical Society
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/http://mnras.oxfordjournals.org/content/451/4/3473.abstract
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1093/mnras/stv1188
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stv1188
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/http://arxiv.org/abs/1506.00554
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/arxiv/1506.00554
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