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Table 4.

Photospheric properties from the X-shooter spectra fit with ROTFIT for the targets in the Orion OB1 Association and σ-Orionis cluster.

Name HJD Teff log g v sin i RV r620 r710 r970
2 459 100+ [K] [km s−1] [km s−1]
CVSO 17 88.62128 3588 ± 22 4.78 ± 0.24 < 6.0 27.4 ± 1.9 0.4 0.2 0.1
CVSO 36 86.62703 3515 ± 24 4.58 ± 0.14 < 6.0 18.6 ± 1.7 0.4 0.4 0.1
CVSO 58 85.76194 3886 ± 45 4.81 ± 0.21 19.3 ± 1.0 23.2 ± 2.2 1.0 0.2 0.5
CVSO 90 98.56264 3489 ± 32 4.26 ± 0.30 13.0 ± 16.0 23.8 ± 2.7 ... 1.8 1.4
CVSO 107 87.58635 3766 ± 37 4.50 ± 0.11 9.4 ± 2.0 16.1 ± 2.0 0.9 0.2 0.3
CVSO 109 81.65721 3799 ± 53 4.42 ± 0.12 < 6.0 17.8 ± 1.7 0.9 0.3 0.3
CVSO 146 92.58387 4079 ± 80 4.70 ± 0.33 < 6.0 16.9 ± 1.7 0.5 0.7 0.2
CVSO 165 97.58340 4040 ± 73 4.09 ± 0.24 12.4 ± 1.0 26.5 ± 1.8 0.5 0.6 0.3
CVSO 176 85.68282 3490 ± 62 4.21 ± 0.22 17.0 ± 7.0 11.1 ± 1.8 1.4 0.5 0.6

SO 518 85.64623 3978 ± 68 4.42 ± 0.46 7.0 ± 12.0 32.3 ± 2.4 1.0 0.9 1.3
SO 583 85.66222 4478 ± 157 4.26 ± 0.33 7.0 ± 8.0 30.9 ± 1.8 1.0 1.3 1.3
SO 1153 90.70681 4086 ± 63 3.92 ± 1.02 13.0 ± 6.0 35.0 ± 2.2 4.2 2.4 2.1

Notes. The measured veiling at different wavelengths is reported in the column labelled ‘r’ followed by the wavelength in nm. We estimate uncertainties of 0.1−0.2 for r < 1.5 and 0.3−0.4 for larger values.

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