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Table A.1

Example of results of photometric inversion of Gaia DR3 data for a few objects among those analysed in this paper.

Number nobs λpole(º) βpole(º) Period (h) b/a c/a k (mag/º) residuals (mag)
16 31 33.77 10.59 8.39145 0.73 0.54 0.0298 0.026256
32 38 103.38 35.28 9.44762 0.75 0.69 0.0281 0.031280
45 30 117.79 27.03 −5.69914 0.71 0.48 0.0408 0.023016
48 50 290.97 38.25 11.88975 0.73 0.65 0.0371 0.037195
55 36 52.34 27.58 4.80404 0.77 0.56 0.0282 0.030328
60 38 273.66 46.48 37.04677 0.74 0.41 0.0283 0.028434
63 34 123.11 33.60 −9.29758 0.53 0.46 0.0392 0.043604
66 37 155.22 89.16 −9.73570 0.79 0.20 0.0379 0.034600
72 37 274.54 57.84 −8.09031 0.77 0.50 0.0386 0.040000
79 57 46.69 18.10 11.98839 0.77 0.72 0.0289 0.022865
82 31 170.94 30.73 −13.00056 0.66 0.65 0.0259 0.028392
95 39 150.46 42.21 8.70223 0.76 0.62 0.0428 0.028750
130 30 268.55 77.70 −5.22461 0.71 0.63 0.0397 0.025272
370420 40 279.94 61.84 −67.05206 0.66 0.38 0.0426 0.047704
374044 28 43.82 39.23 461.48373 0.59 0.15 0.0333 0.027286
376764 35 194.85 54.87 1458.21077 0.53 0.23 0.0217 0.025372
391082 35 94.58 49.68 −4.80448 0.25 0.15 0.0434 0.026300
391532 25 315.25 35.64 138.67156 0.75 0.58 0.0308 0.041058
393373 35 72.34 14.99 −3.40214 0.38 0.38 0.0274 0.029245

Notes. Only inversion solutions passing the filter described in Section 3.1 are shown. The full Table is available at the Centre de Données astronomiques de Strasbourg (CDS)6

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