Physical parameters of stars derived by SPIPS at Spitzer observation phase.
|Teff (ϕSpitzer)||log g(ϕSpitzer)||θ(ϕSpitzer)|
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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