J/A+A/665/A66       Calern Asteroid Polarisation Survey        (Bendjoya+, 2022)

The Calern Asteroid Polarisation Survey: An updated catalogue of asteroid polarimetric data. Bendjoya P., Cellino A., Rivet J.-P., Devogele M., Bagnulo S., Abe L., Vernet D., Gil-Hutton R., Venezian A. <Astron. Astrophys. 665, A66 (2022)> =2022A&A...665A..66B 2022A&A...665A..66B (SIMBAD/NED BibCode)
ADC_Keywords: Minor planets Keywords: minor planets - asteroids: general - catalogs Abstract: The Calern Asteroid Polarimetric Survey (CAPS), a collaboration between the INAF Astrophysical Observatory of Torino (Italy) and the Observatoire de la Cote 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. 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. 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. 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. 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. Description: The Calern Asteroid Polarimetric Survey (CAPS), a collaboration between the INAF, Astrophysical Observatory of Torino (Italy) and the Observatoire de la Cote 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. 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 polarimetric properties. Until now unpublished data, from the CASLEO (Complejo Astronomico El Leoncito) survey are also added to the catalogs. The CAPS catalog includes the results obtained by the Calern Asteroid Polarimetric Survey since the beginning of operations (August, 2018), up to December, 2021. All the data collected for each object are listed, specifying for each entry the object's identification number, the epoch of observation (expressed as year, month, day and fraction of day, the phase angle, the value of the measured Pr, its error, and the filter used. As for the latter, it is most commonly the standard V filter, but in several cases also the B, R and I filters of the Johnson-Cousin system have been used. The CASLEO catalog lists, using the same format adopted for the CAPS data, a number of unpublished polarimetric measurements of asteroids obtained between 1995 and 2004, plus a small number of measurements obtained in 2013, using the 2.15m telescope of the Complejo Astronomico El Leoncito (CASLEO), managed by the Universities of La Plata, Cordoba and San Juan (Argentina), and the Argentinian scientific and technical research council (CONICET).The U, B, V, R and I filters are those of the Johnson-Cousin system. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file list.dat 35 600 List of asteroids with data in tables caps.dat 67 2050 The CAPS data (table A1) casleo.dat 67 1129 The CASLEO data (table A2) -------------------------------------------------------------------------------- See also: B/astorb : Orbits of Minor Planets (Bowell+ 2014-) Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- Id Asteroid number 8- 27 A20 --- Name Asteroid name 29- 30 I2 --- NT1 ? Number of measurements in CAPS data (table A1) 34- 35 I2 --- NT2 ? Number of measurements in CASLEO data (table A2) -------------------------------------------------------------------------------- Byte-by-byte Description of file: caps.dat casleo.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 5- 10 I6 --- Id Asteroid Identification 17- 26 A10 "date" Date Observation date, YYYY-MM-DD 31- 35 F5.3 d Frac Fraction of the Day 39- 44 F6.2 deg alph Phase angle 49- 53 F5.2 % Pr Linear degree of Polarisation 58- 62 F5.2 % e_Pr Error on Linear degree of Polarisation 67 A1 --- Filter [UBVRI] Filter UBVRI in Johnson-Cousin system ------------------------------------------------------------------------------- Acknowledgements: Philippe Bendjoya, bendjoya(at)oca.eu, Univ. Cote d'Azur-Obs. Cote d'Azur-CNRS
(End) Philippe Bendjoya [Obs. Cote d'Azur], Patricia Vannier [CDS] 05-Sep-2022
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line