Table 1.
Parameters for our diffuse Galactic emission angular power spectrum model.
| Component | Polarisation | A(K2) | α | β | ζ |
|---|---|---|---|---|---|
| Galaxy | TT | 0.0028 | 2.2 | 2.55 | 4.0 |
Notes. The angular power spectrum model is given in Equation (1). The parameters are based on the models of Santos et al. (2005) and informed by LOFAR-AARTFAAC data of the NCP (Gehlot et al. 2022). TT refers to the temperature-temperature power spectrum.
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