bbflux

sofia_redux.calibration.standard_model.thermast.bbflux(omega, tss, w)[source]

Calculate the modified blackbody flux from the asteroid.

Parameters:
omeganumpy.array

Angular distance from the sub-solar point.

tssfloat

Maximum sub-solar temperature of the asteroid in Kelvins.

wfloat

Wavelength in microns.

Returns:
fluxnumpy.array

Thermal flux as a function of omega.

Notes

This function computes the integrand of Equation 10 from Delbo & Harris (2002).