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Table 1.

Observations log, radial velocities and stellar parameters for VX Sgr.

Date BJD Instrument texp RV Teff ζ SpT
Remark
[s] [km s−1] [K] [km s−1] Optical Near-infrared
2016-04-04 2457482 SES 3600 −4.3 ± 0.2 3408 ± 37 4.19 ± 0.36 M7 M8 Rb double lined
2016-05-21 2457529 SES 3600 −4.5 ± 0.2 3360 ± 32 4.72 ± 0.54 M8 M8.5 Rb double lined
2016-09-22 2457653 SES 6000 −5.0 ± 0.4 3523 ± 25 6.87 ± 0.32 M5.5 M7 H in emission
2016-10-25 2457686 UVES 10.5 −4.9 ± 0.2 3471 ± 13 9.19 ± 0.86 M4.5 M7
2017-02-12 2457796 UVES 2.5 −5.2 ± 0.1 3318 ± 10 10.18 ± 0.80 M5.5 M7.5
2017-03-04 2457816 UVES 8.5 −5.2 ± 0.1 3261 ± 68 10.36 ± 0.90 M5.5 M7.5
2017-04-02 2457845 SES 3000 −4.7 ± 0.2 3347 ± 24 6.54 ± 0.55 M6 M8
2017-05-17 2457890 SES 3000 −4.3 ± 0.2 3273 ± 29 6.26 ± 0.50 M6 M8
2017-06-29 2457933 SES 3000 −4.1 ± 0.2 3294 ± 37 6.49 ± 0.56 M6.5 M8
2017-08-06 2457971 SES 6000 −3.6 ± 0.2 3272 ± 36 5.36 ± 0.75 M7 M8.5
2018-06-06 2458275 SES 3000 −3.3 ± 0.3 3562 ± 19 6.24 ± 0.38 M3 M4 H in emission; doubled atomic lines

Notes. The table lists: epochs of observation, instrument used to acquire each observation, total exposure times for each epoch (texp), radial velocities (RV), Specral types (SpT), and physical parameters for VX Sgr (Teff, ζ). log g is fixed to −0.5 dex whereas [M/H] is also fixed to 0.0 dex (see text for details). The accuracy of the spectral classification is one subtype.

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