def _planck(self, lam, Teff):
"""
Computes monochromatic blackbody intensity in W/m^3 using the
Planck function.
@lam: wavelength in m
@Teff: effective temperature in K
Returns: monochromatic blackbody intensity
"""
return 2*self.h*self.c*self.c/lam**5 * 1./(np.exp(self.h*self.c/lam/self.k/Teff)-1)
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