Table 3
Spectroscopic and photometric datasets used for the bolometric flux computation with the corresponding spectral ranges.
Target | INES | TD1 | Adelman (+) | Visible | 2MASS | fbol [erg cm−2 s−1] | fbol [erg cm−2 s−1] |
---|---|---|---|---|---|---|---|
spectra | This work | from modelling | |||||
HD 4778 | [1265 ... 3180] | Y | – | [3900 ... 6800] (a) | J, H, K | 0.97 ± 0.10 ×10−7 | – |
HD 108662 | [1265 ... 3180] | – | [3300 ... 7100] | [4000 ... 6800] (a) | J, H, K | 2.24 ± 0.21× 10−7 (•) | 2.53 ± 0.15 × 10−7 |
HD 108945 | [1265 ... 3180] | Y | [3300 ... 7100] | [3900 ... 6800] (a) | J, H, K | 1.68 ± 0.15 × 10−7 | – |
HD 120198 | [1265 ... 3180] | Y | [3300 ... 7100] | [3725 ... 7210] (b) | J, H, K | 1.62 ± 0.13 × 10−7 | – |
HD 153882 | – | Y | [3390 ... 7850] | [3535 ... 7405](c) | J, H, K | 0.81 ± 0.06× 10−7 | 0.79 ± 0.04 × 10−7 |
HD 188041 | [1977 ... 3180] | Y | [3390 ... 7850] | [3535 ... 7405] (c) | J, H, K | 1.34 ± 0.16 × 10−7 | 1.34 ± 0.25 ×10−7 |
HD 204411 | – | Y | [3300 ... 6800] | [3720 ... 7215] (b) | J, H, K | 1.90 ± 0.15× 10−7 | 1.84 ± 0.15 ×10−7 |
HD 220825 | – | – | [3300 ... 7850] | [3725 ... 7215] (b) | J, H, K | 2.30 ± 0.17 ×10−7 | – |
Notes. The bolometric fluxes obtained from our work and from self-consistent atmosphere modelling are given in the last two columns. See text for details. (+) Adelman data are photometric values collected over the optical range. Visible spectra: (a) ELODIE; (b) OAN; (c) MILES. (∙) We accounted for the 1.32 scale factor of the IUE flux, as explained in Sect. 3.1.
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