CMBMap¶
- class pysm3.CMBMap(nside, max_nside=None, map_IQU=None, map_I=None, map_Q=None, map_U=None, map_dist=None)[source] [edit on github]¶
Bases:
Model
Load one or a set of 3 CMB maps
The input is assumed to be in
uK_CMB
- Parameters:
- nside: int
HEALPix N_side parameter of the input maps
- map_IQU: `pathlib.Path` object
Path to a single IQU map
- map_I, map_Q, map_U: `pathlib.Path` object
Paths to the maps to be used as I, Q, U templates.
Methods Summary
get_emission
(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(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: scalar or array astropy.units.Quantity
Frequency at which the model should be evaluated, in a frequency which can be converted to GHz using astropy.units. If an array of frequencies is provided, integrate using trapz with a equal weighting, i.e. simulate a top-hat bandpass.
- weights: np.array, optional
Array of weights describing the frequency response of the instrument, i.e. the bandpass. Weights are normalized and applied in Jy/sr.
- Returns:
- outputastropy.units.Quantity
Simulated map at the given frequency or integrated over the given bandpass. The shape of the output is (3,npix) for polarized components, (1,npix) for temperature-only components. Output is in
uK_RJ
.