integrate_sed¶

dust_emissivity.blackbody.integrate_sed(vmin, vmax, function=<function blackbody>, **kwargs)[source]¶

Integrate one of the SED functions over frequency

Parameters:

vmin, vmax : astropy.Quantity

Quantities with frequency equivalents: can be wavelength or frequency

function : function

One of the above blackbody functions. The temperature etc. can be specified with kwargs

Returns:

The SED integrated in units of

bbunit = u.erg/u.s/u.cm**2