SpDustPol

class pysm.SpDustPol(map_I, freq_ref_I, emissivity, freq_peak, freq_ref_peak, pol_frac, angle_Q, angle_U, nside, unit_I=None, map_dist=None)[source] [edit on github]

Bases: pysm.SpDust

SpDust2 model with Polarized emission

This function initializes the spinning dust model

Parameters
map_Ipathlib.Path object

Paths to the map to be used as I templates.

unit_Istring or Unit

Unit string or Unit object for all input FITS maps, if None, the input file should have a unit defined in the FITS header.

freq_ref_IQuantity or string

Reference frequencies at which the templates are defined. They should be a astropy Quantity object or a string (e.g. “1500 MHz”) compatible with GHz.

freq_peakpathlib.Path object or string

Path to the map to be used as frequency of the peak of the emission or its scalar value as a Quantity or a string convertible to a Quantity

freq_ref_peakQuantity or string

Reference frequency for the peak frequency map They should be a astropy Quantity object or a string (e.g. “1500 MHz”) compatible with GHz.

nside: int

Resolution parameter at which this model is to be calculated.

Methods Summary

get_emission(self, freqs[, weights])

This function evaluates the component model at a either a single frequency, an array of frequencies, or over a bandpass.

Methods Documentation

get_emission(self, freqs:Unit("GHz"), weights=None)[source] [edit on github]

This function evaluates the component model at a either a single frequency, an array of frequencies, or over a bandpass.

Parameters
freqs: float

Frequency at which the model should be evaluated, assumed to be given in GHz.

Returns
ndarray

Set of maps at the given frequency or frequencies. This will have shape (nfreq, 3, npix).