flux_at_w

sofia_redux.calibration.standard_model.thermast.flux_at_w(warr, subsolar_temperature, omin=0.0, omax=1.5707963267948966)

Calculate the thermal flux from a blackbody object.

Parameters:

warrnumpy.array

Wavelengths to calculate flux at, in microns.

subsolar_temperaturefloat

Maximum sub-solar temperature of the asteroid, as given by Equation 9 in Deblo & Harris (2002).

ominfloat, optional

Lower omega limit of integration in radians. Defaults to 0.

omaxfloat

Upper omega limit of integration in radians. Defaults to $pi$/2.

Returns:

fluxnumpy.array

Wavelength dependent component of the blackbody flux of the object.

Notes

Implementation of the integral in Equation 10 from Delbo & Harris (2002).

\[F_{\lambda} \,=\, \int_{\Omega_{min}}^{\Omega{\max}} d\Omega\]