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J/A+A/642/A180
  Hot subdwarf stars binarity (Pelisoli+, 2020)
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    J/A+A/642/A180/table1(c)61 variables in our sample whose variability was attributed to rotation of the main sequence companion, identified by their TESS Input Catalogue (TIC) numbers (61 rows)
    J/A+A/642/A180/table2(c)27 objects whose cause for variability is undetermined (27 rows)
    J/A+A/642/A180/table3(c)Systems for which no periodic variability has been detected (33 rows)
    J/A+A/642/A180/table4(c)Identified common proper motion candidates (16 rows)

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       (c)  indicates tables which contain celestial coordinates 
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