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Table 3

Properties of the calibrators for the VLTI/MATISSE and GRAVITY observations.

Name Spectral type LDD diameter (mas) Teff (K) log 𝑔 [Z]
gam02 Nor K0III 2.46 ± 0.25 4750 3.0 0.25
eps Sco K1III 5.93 ± 0.45 4500 2.5 −0.25
nu Oph K1III 2.83 ± 0.29 5000 3.0 0.00
HD 94683 K4III 2.49 ± 0.25 4000 0.0 0.00
HD 91056 M0III 4.40 ± 0.49 3800 1.0 0.00
HD 16074 K2III 1.77 ± 0.13 4250 −0.5 0.00
ups Cet M0III 5.91 ± 0.76 3800 1.15 −0.05
HD 302821 A7Ie 1.26 ± 0.10 3700 0.00 0.00
zet Vol K0III 2.23 ± 0.21 4700 2.5 −0.2
CD-55 3254 M3 2.76 ± 0.27 3300 0.00 0.00
HD 159881 K5III 2.81 ± 0.24 4500 2.5 −0.25
HD 152636 K5III 2.39 ± 0.22 4000 2.5 −0.05
HD 96442 M1/2III 1.64 ± 0.16 4000 0.00 0.00
HD 103859 K4III 1.43 ± 0.11 4000 0.00 0.00
80 Cet M0III 3.57 ± 0.36 4000 0.00 0.00
HD 89736 K5/M0III 2.58 ± 0.23 3900 0.00 0.00
HD 90677 K3II 1.99 ± 0.19 4000 0.00 0.00
Q Car K3III 2.45 ± 0.27 4300 0.00 0.00
HD 60228 M1III 2.51 ± 0.24 3900 0.00 0.00

Notes. Shown are the name, spectral type, limb-darkened disk diameter (LDD) from Bourges et al. (2017), and the stellar parameters of the synthetic spectra (MARCS, Gustafsson et al. 2008) used for the calibrators: effective temperature (Teff), surface gravity (log 𝑔), and metallicity [Z] available in the VizieR database of astronomical catalogues (Ochsenbein et al. 2000).

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