conv_bps module

Collect all 3x2pt observed spectra (pseudo-Cl bandpowers) into one file for input into inference code

pcl_measurement.conv_bps.conv_1x2pt_bps(n_zbin, n_bp, save_dir, recov_cat_bps_path, obs_type='obs', field='E')

Collect all Pseudo bandpowers for a tomographic 1x2pt (shear only or clustering only) and store into single array.

Parameters

n_zbin(float): Number of tomographic redshift bins
n_bp(float): Number of bandpowers
save_dir(str): Path to directory that stores all measurement data (MEASUREMENT_SAVE_DIR from the set_variables_3x2pt_measurement.ini file)
recov_cat_bps_path(str): Location to store combined 1x2pt data vector as .npz file
obs_type(str): Use the data measured from simulation (‘obs’) or the fiducial data (‘fid’) to generate the combined data vector
field(str): ‘E’ or ‘N’ to specify the 1x2pt measurement is cosmic shear only or angular clustering only

Saves array in .npz format of the combined 3x2pt data vector.

pcl_measurement.conv_bps.conv_3x2pt_bps(n_zbin, n_bp, save_dir, recov_cat_bps_path, obs_type='obs')

Collect all 3x2pt tomographic Pseudo bandpowers and store into single array.

n_zbin(float): Number of tomographic redshift bins
n_bp(float): Number of bandpowers
save_dir(str): Path to directory that stores all measurement data (MEASUREMENT_SAVE_DIR from the set_variables_3x2pt_measurement.ini file)
recov_cat_bps_path(str): Location to store combined 3x2pt data vector as .npz file
obs_type(str): Use the data measured from simulation (‘obs’) or the fiducial data (‘fid’) to generate the combined data vector

Saves array in .npz format of the combined 3x2pt data vector.

pcl_measurement.conv_bps.main(): Main function to generate combined 3x2pt or 1x2pt joint tomographic data vector

pcl_measurement.conv_bps.mysplit(s)

Function to split string into float and number. Used to extract which field and which tomographic bin should be identified and collected.