Table A.1
Calibrator observed and used to reduce the data.
| Calibrator’s name | Diameter [mas] | Error [mas] | Science target | Observing dates |
|---|---|---|---|---|
| 2MASS J19524977+4836263 | 0.46 | 0.03 | HD 188209 | 2018-06-09 |
| 2MASS J20295613+4137570 | 0.31 | 0.01 | Cyg OB2-9 | 2018-09-23 |
| … | … | … | HD 193322 | 2018-06-12 |
| … | … | … | HD 34078 | 2017-12-13 |
| 2MASS J20473119+3629045 | 0.2 | 0.01 | HD 201345 | 2019-06-27 |
| 2MASS J21281481+6005284 | 0.52 | 0.03 | HD 209975 | 2018-06-09 |
| HD 21820 | 0.48 | 0.03 | HD 24534 | 2018-09-23, 2018-09-27 |
| HD 22269 | 0.58 | 0.03 | HD 24534 | 2018-09-27 |
| HD 24688 | 0.37 | 0.03 | HD 24431 | 2018-09-24 |
| HD 26311 | 1.64 | 0.03 | HD 24534 | 2018-02-08 |
| HD 30111 | 0.562 | 0.03 | HD 34078 | 2017-12-13 |
| HD 30793 | 0.53 | 0.03 | HD 34078 | 2018-09-23, 2018-09-27 |
| HD 32518 | 0.816 | 0.03 | HD 30614 | 2018-09-25 |
| HD 35238 | 1.03 | 0.05 | HD 34078 | 2018-09-27 |
| HD 42618 | 0.377 | 0.03 | HD 34078 | 2017-12-13 |
| HD 45089 | 0.61 | 0.03 | HD 41129 | 2018-09-23, 2018-09-24 |
| … | … | … | HD 45314 | 2018-09-25 |
| HD 46714 | 0.86 | 0.03 | HD 47432 | 2018-09-27 |
| HD 48596 | 0.53 | 0.03 | HD 47432 | 2018-09-26, 2018-09-27 |
| HD 49019 | 0.89 | 0.03 | HD 36861 | 2018-02-07 |
| HD 52961 | 0.232 | 0.02 | HD 34078 | 2017-12-13 |
| HD 77250 | 0.8 | 0.04 | HD 34078 | 2017-12-13 |
| HD 87828 | 0.78 | 0.03 | HD 89353 | 2018-02-07 |
| HD 150470 | 0.45 | 0.01 | HD 150193* | 2019-06-24 |
| HD 155524 | 0.49 | 0.03 | Cyg OB2-5 A | 2018-06-10 |
| … | … | … | HD 157214* | 2018-06-11 |
| HD 165480 | 0.44 | 0.01 | HD 166737 | 2019-06-24 |
| HD 185663 | 0.64 | 0.03 | HD 188001 | 2018-09-26 |
| HD 186962 | 0.41 | 0.01 | HD 188001 | 2018-09-26 |
| HD 189942 | 1.15 | 0.05 | HD 193237* | 2018-06-24 |
| HD 193217 | 1.57 | 0.03 | Cyg OB2-5 A | 2018-06-10 |
| HD 195647 | 0.42 | 0.03 | HD 229196 | 2018-09-24 |
| … | … | … | Cyg OB2-9 | 2018-09-27 |
| … | … | … | Cyg OB2-8 | 2018-06-12 |
| Cyg OB2-10 | 2019-06-23 | |||
| HD 196134 | 0.71 | 0.06 | Cyg OB2-5 A | 2019-06-23 |
| HD 196360 | 0.6 | 0.03 | Cyg OB2-9 | 2018-09-24 |
| … | … | … | HD 229196 | 2018-09-27 |
| HD 200060 | 0.516 | 0.03 | Cyg OB2-11 | 2018-09-25 |
| HD 204050 | 0.42 | 0.03 | HD 203064 | 2018-06-10 |
| HD 204721 | 0.6 | 0.06 | HD 207198 | 2019-06-24 |
| HD 211982 | 0.57 | 0.02 | HD 202214 | 2018-06-09 |
| … | … | … | HD 210839 | 2018-06-09 |
| HD 212289 | 0.48 | 0.03 | HD 203064 | 2018-06-10 |
| … | … | … | HD 214686 | 2018-06-11 |
| HD 217711 | 0.67 | 0.03 | HD 2018086 | 2018-09-26 |
| HD 228660 | 0.58 | 0.01 | HD 228779 | 2019-06-26 |
| HD 228721 | 0.31 | 0.01 | HD 229202 | 2019-06-27 |
| HD 228852 | 0.54 | 0.03 | Cyg OB2-9 | 2018-09-24 |
| … | … | … | HD 193322 | 2018-09-27, 2019-06-24 |
| HD 232948 | 0.68 | 0.03 | HD 36861 | 2018-02-08 |
| … | … | … | HD 28446 | 2018-09-24 |
| HD 235757 | 0.43 | 0.01 | HD 210809 | 2019-06-26 |
| HD 235872 | 0.34 | 0.01 | HD 218915 | 2019-06-27 |
| HD 237032 | 0.76 | 0.03 | HD 17505 | 2018-09-25, 2018-09-26 |
| HD 237036 | 0.5 | 0.03 | HD 17505 | 2018-09-26 |
| HD 239636 | 0.36 | 0.01 | HD 202214 | 2018-06-09, 2019-06-24 |
| HD 239760 | 0.61 | 0.02 | HD 206267 | 2019-06-22 |
| HD 240211 | 0.34 | 0.03 | HD 217086 | 2018-09-26 |
| HD 246454 | 0.6 | 0.03 | HD 36861 | 2018-09-26 |
| HD 254874 | 0.51 | 0.03 | HD 45314 | 2018-02-07 |
| HD 261683 | 0.56 | 0.03 | HD 47839 | 2018-09-25 |
| SAO 50079 | 0.4 | 0.03 | Cyg OB2-10 | 2018-06-12 |
| SAO 50138 | 0.38 | 0.03 | HD 199579 | 2018-06-11 |
| SAO 50258 | 0.27 | 0.03 | LS III +46 11 | 2018-06-24 |
Notes. The first column is the calibrator name. The second column is the diameter of the calibrator in the H-band in mas as stated in the JSDC catalog (Bourges et al. 2017). The third column is the associated error in mas. The fourth column is the science target it has calibrated. The fifth column gives the observing dates at which the calibrator was used for this science target. We note that science targets noted with the symbol * are non O-type stars observed during the observing runs: their calibrators were still used for the data reduction. Concerning O-type star science targets present in this table that were observed with the associated calibrator, but had not good enough quality data, thus them not being present in the results, their calibrator was still used for the data reduction.
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