Table 1
HD 113337 VEGA observation and reduction log.
Date | Calibrator | ![]() |
![]() |
UT | Calibration | λobs | Baseline | BP | PA | V2 | r0 |
---|---|---|---|---|---|---|---|---|---|---|---|
(HD) | (mas) | (mas) | (on target) | sequence | (nm) | (m) | (°) | (cm) | |||
2013-05-25 | 111270 (C1) | 0.307 | 0.021 | 04:35 | C1-S-C1 | 730 | E2W1 | 250 | −131 | 0.321 ± 0.040 | 9 |
110462 (C2) | 0.221 | 0.014 | 710 | E2W1 | 250 | −131.5 | 0.357 ± 0.046 | ||||
06:23 | C1-S-C2 | 750 | E2W1 | 249 | −100 | 0.420 ± 0.048 | |||||
730 | E2W1 | 249 | −100 | 0.323 ± 0.032 | |||||||
710 | E1E2 | 64 | −121 | 0.818 ± 0.052 | |||||||
710 | E2W1 | 249 | −100 | 0.362 ± 0.042 | |||||||
2014-07-03 | 98772 | 0.230 | 0.014 | 04:32 | C-S-C | 710 | E2W2 | 156 | −176 | 0.780 ± 0.058 | 8 |
700 | E2W2 | 156 | −176 | 0.708 ± 0.053 | |||||||
2014-07-07 | 98772 | 0.230 | 0.014 | 04:17 | C-S-C | 710 | E2W2 | 156 | 174 | 0.650 ± 0.051 | 6 |
700 | E2W2 | 156 | 174 | 0.648 ± 0.052 | |||||||
2015-05-30 | 118214 | 0.230 | 0.015 | 06:01 | C-S-C | 710 | E2W2 | 156 | −141 | 0.712 ± 0.023 | 7 |
700 | E2W2 | 156 | −141 | 0.658 ± 0.020 | |||||||
2015-06-01 | 121409 | 0.226 | 0.015 | 06:02 | C-S-C | 710 | E1E2 | 66 | −151 | 0.914 ± 0.018 | 10 |
710 | E2W1 | 245 | −130 | 0.510 ± 0.070 | |||||||
700 | E1E2 | 66 | −151 | 0.902 ± 0.017 | |||||||
06:45 | C-S-C | 710 | E1E2 | 66 | −148 | 0.940 ± 0.018 | |||||
700 | E1E2 | 66 | −148 | 0.918 ± 0.017 | |||||||
Notes. Only the selected V2 measurements (see text) are listed. Columns 1 and 5 give the observation date and UT time (on the science target). Columns 2–4 give the calibrator identifier in the HD catalogue, its uniform-disc angular diameter () in the R band, and the 1σ error bar on the calibrator diameter (
). We took the calibrator diameters from the JMMC Stellar Diameters Catalog Version 2 (JSDC; Bourges et al. 2017), while we kept the corresponding 1σ uncertainties from the JSDC Version 1 (Lafrasse et al. 2010, see text). Column 6 gives the calibration sequence followed for the observation and Col. 8 is the baseline used. Column 7 gives the central wavelength of the 20-nm-wide spectral bands in which we computed the V2. Columns 9 and 10 give the projected base length BP and its orientation PA. Column 11 gives the corresponding calibrated V2 value. Column 12 gives the Fried parameter (estimation of the quality of the atmosphere) for each observation night. We note that three observation points are not listed as the results were fully rejected (see text).
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