The Calern Asteroid Polarisation Survey

An updated catalogue of asteroid polarimetric data^★

¹ Côte d’Azur University, Côte d’Azur Observatory, CNRS, Lagrange Laboratory, Valsros Campus, 06108 Nice Cedex 02, France
e-mail: philippe.bendjoya@unice.fr
² INAF, Osservatorio Astrofisico di Torino, via Osservatorio 20, 10025 Pino Torinese, Italy
e-mail: alberto.cellino@inaf.it
³ Lowell Observatory, 1400 W. Mars Hill Road, Flagstaff, AZ 86001, USA
⁴ Armagh Observatory and Planetarium, College Hill, Armagh BT61 9DG, UK
⁵ Grupo de Ciencias Planetarias, Departamento de Geofísica y Astronomía, Facultad de Ciencias Exactas, Físicas y Naturales, Universidad Nacional de San Juan – CONICET, Av. J. I. de La Roza 590 Oeste, J5402DCS Rivadavia, San Juan, Argentina
⁶ Physics department, Torino University, via Pietro Giuria 1, 10025 Torino, Italy

Received: 20 December 2021
Accepted: 13 June 2022

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.