CMM.preset.preset_sky module

class CMM.preset.preset_sky.PresetSky(preset_tools, preset_qubic)[source]

Bases: object

Preset Sky.

Instance to initialize the Components Map-Making. It defines the observed sky variables and methods.

Parameters:

preset_tools (object) – Class containing tools and simulation parameters.
preset_qubic (object) – Class containing qubic operator and variables and methods.

center

Defines the center of the QUBIC observation patch in (RA, DEC).

Type:: tuple

coverage

Defines the coverage of the QUBIC scanning strategy.

Type:: array_like

max_coverage

Defines the maximum of the coverage.

Type:: float

seenpix_qubic

Boolean array defining the pixels seen by QUBIC instrument.

Type:: array_like

seenpix

Boolean array defining the pixel with coverage > at a threshold chosen in params.yml.

Type:: array_like

namaster

NaMaster class instance.

Type:: object

ell

Multipole array, defining through NaMaster.

Type:: array_like

cl2dl

Array containing conversion factor to compute \(D_{\ell}\) from \(C_{\ell}\).

Type:: array_like

Methods

`get_coverage`()	Coverage.
`get_spectra_namaster_informations`()	NaMaster.

get_coverage()[source]

Coverage.

Calculate the coverage mask for the QUBIC patch, according with the number of beta that you want to reconstruct.

This function computes the angular distance between a center point and all pixels on a sphere, sorts these distances, and creates a mask that marks the closest pixels as covered.

Returns:: mask – A mask array where covered pixels are marked with 1 and uncovered pixels are marked with 0.
Return type:: array_like

get_spectra_namaster_informations()[source]

NaMaster.

Initializes the Namaster object and computes the ell and cl2dl arrays.

This method sets up the Namaster object using parameters from the preset_tools and computes the ell array and cl2dl conversion factor for power spectrum analysis.