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Table A.1

List of CAPS polarimetric measurements

Asteroid Number Date of observation Fraction of day Phase angle (deg) Pr (%) Filter
1 2016-08-17 0.073 19.00 0.16 ± 0.09 V
1 2016-08-18 0.071 18.89 0.15 ± 0.09 V
1 2016-08-21 0.018 18.53 0.01 ± 0.09 V
1 2016-08-22 0.108 18.39 0.03 ± 0.09 V
1 2016-12-01 0.867 15.24 −0.83 ± 0.08 V
1 2016-12-05 0.848 16.15 −0.59 ± 0.12 V
1 2017-12-19 0.248 17.02 −0.23 ± 0.09 V
1 2018-01-12 0.034 9.53 −1.40 ± 0.09 V
1 2018-05-08 0.892 23.12 1.40 ± 0.09 V
1 2021-08-22 0.142 20.85 0.69 ± 0.08 V
2 2016-08-17 0.948 7.05 −1.47 ± 0.10 V
2 2016-08-18 0.926 6.99 −1.53 ± 0.09 V
2 2016-12-02 0.721 16.96 −0.34 ± 0.08 V
2 2015-02-18 0.191 18.70 0.05 ± 0.08 V
2 2015-02-18 0.191 18.70 0.08 ± 0.08 R
2 2016-07-19 0.048 12.24 −1.21 ± 0.08 V
2 2019-01-28 0.246 24.05 1.32 ± 0.08 V
2 2019-02-11 0.196 22.17 0.86 ± 0.08 V
2 2019-04-08 0.995 10.61 −1.42 ± 0.08 V
2 2020-02-24 0.228 15.09 −0.67 ± 0.08 V
2 2020-04-06 0.182 17.67 −0.04 ± 0.10 V
2 2020-04-07 0.175 17.69 −0.16 ± 0.09 V
2 2020-05-08 0.132 17.20 −0.43 ± 0.08 V
2 2021-08-13 0.054 10.61 −1.55 ± 0.08 V
2 2021-12-02 0.739 19.23 0.10 ± 0.08 V
3 2015-02-18 0.941 11.91 −0.62 ± 0.08 V
3 2015-02-18 0.941 11.91 −0.66 ± 0.08 R
3 2016-06-01 0.892 12.05 −0.57 ± 0.08 V
3 2017-07-06 0.888 6.08 −0.48 ± 0.08 V
3 2017-07-27 0.842 10.71 −0.69 ± 0.08 V
3 2017-07-29 0.930 11.27 −0.67 ± 0.08 V
3 2017-08-12 0.877 14.77 −0.56 ± 0.09 V
3 2020-02-18 0.144 15.13 −0.45 ± 0.10 V
3 2020-04-10 0.029 4.16 −0.63 ± 0.08 V
3 2021-04-19 0.150 14.35 −0.58 ± 0.09 V
4 2016-12-01 0.116 18.90 −0.20 ± 0.09 V
4 2018-03-19 0.212 27.43 0.36 ± 0.10 V
4 2018-03-21 0.189 27.41 0.17 ± 0.08 V
4 2018-03-22 0.185 27.39 0.26 ± 0.08 V
4 2018-05-23 0.057 14.21 −0.48 ± 0.08 V
4 2019-10-07 0.127 15.70 −0.43 ± 0.08 V
4 2019-10-09 0.088 15.05 −0.43 ± 0.08 V
4 2020-01-07 0.888 20.29 −0.20 ± 0.08 V
4 2021-01-11 0.136 20.68 −0.14 ± 0.08 V
4 2021-03-01 0.005 4.69 −0.61 ± 0.08 V
5 2016-06-08 0.883 27.22 0.79 ± 0.10 V

Notes. A short sample of the results obtained by the Calern Asteroid Polarimetric Survey, since the beginning of operations and up to December 2021. The whole data table has been uploaded to the Centre de Données astronomiques de Strasbourg (CDS) (http://cdsads.u-strasbg.fr/). All the observations 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. A few additional measurements in BRI colours taken since 2018 are not listed because they are still under reduction.

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