Table 3
Physical parameters of stars derived by SPIPS at Spitzer observation phase.
| Teff (ϕSpitzer) | log g(ϕSpitzer) | θ(ϕSpitzer) | ||
|---|---|---|---|---|
| RS Pup |  |
 |
 |
|
| ζ Gem |  |
 |
 |
|
| η Aql |  |
 |
 |
|
| V Cen |  |
 |
 |
|
| SU Cyg |  |
 |
 |
|
Notes. Teff and log g are used to interpolate a ATLAS9 atmosphere model. The limb-darkened angular diameter θ is then used to derived the observed flux. Temperature and angular diameter are in Kelvin and milliarcsecond respectively. Uncertainties on Teff and θ are provided by SPIPS, whereas uncertainty on log g is arbitrarily set to 10%.
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