Table D.1.
Magnitudes of non-accreting stars scaled to a radius of R⊙ and a distance of 403 pc as a function of Teff.
| Teff [K] | u′ [mag] | g′ [mag] | r′ [mag] |
|---|---|---|---|
| 5835 |
 |
 |
 |
| 5669 |
 |
 |
 |
| 5505 |
 |
 |
 |
| 5339 |
 |
 |
 |
| 5174 |
 |
 |
 |
| 5010 |
 |
 |
 |
| 4845 |
 |
 |
 |
| 4680 |
 |
 |
 |
| 4514 |
 |
 |
 |
| 4350 |
 |
 |
 |
| 4184 |
 |
 |
 |
| 4019 |
 |
 |
 |
| 3855 |
 |
 |
 |
| 3689 |
 |
 |
 |
| 3525 |
 |
 |
 |
| 3360 |
 |
 |
 |
| 3195 |
 |
 |
 |
| 3029 |
 |
 |
 |
| 2865 |
 |
 |
 |
| 2700 |
 |
 |
 |
Notes. The values describe the best fit of a nonparametric regression and the 95 % confidence interval. The input for the regression was synthetic u′g′r′ photometry of X-Shooter spectra from diskless class III objects observed by Manara et al. (2013, 2017a).
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