Spinning Dust¶
- class cosmoglobe.sky.components.ame.SpinningDust(amp, freq_ref, **spectral_parameters)[source]¶
Class representing the AME component in the Cosmoglobe Sky Model.
Notes
The spinning dust emission is defined using the convention in BeyondPlanck (2020), Section 3.3.4;
\[\boldsymbol{s}_{\mathrm{RJ}}^{\mathrm{sd}}(\nu) \propto \nu^{-2} \boldsymbol{s}_{0}^{\mathrm{sd}}\left(\nu \cdot \frac{30.0\; \mathrm{GHz}}{\nu_{p}}\right)\]where \(\nu\) is the frequency for which we are simulating the sky emission, \(\boldsymbol{s}_0^{\mathrm{sd}}\) is the spdust2 template, and \(\nu_p\) the peak frequency.