Radio¶
- class cosmoglobe.sky.components.radio.AGNPowerLaw(amp, freq_ref, **spectral_parameters)[source]¶
Class representing the radio component.
Notes
This is a generic power law given at a reference frequency \(\nu_{\mathrm{0, src}}\) with a power law spectral index \(\alpha\). It is defined using the convention in BeyondPlanck (2020), Section 3.4.1;
\[\boldsymbol{s}_{\mathrm{RJ}}^{\mathrm{src}}(\nu) \propto \left(\frac{\nu}{\nu_{\mathrm{0, src}}}\right)^{\alpha-2}\]where \(\nu\) is the frequency for which we are simulating the sky emission.