BrahMap quick start guide

Complete example scripts and notebooks can be found here.

By default, BrahMap performs all the operations over global MPI communicator (MPI.COMM_WORLD). To modify this behavior, one can specify a different MPI communicator through the function brahmap.MPI_UTILS.update_communicator(comm=...). This function must be called before calling any other BrahMap functions.

General map-making

A generic map-making using BrahMap roughly involve four steps:

1. Pre-processing the pointing information (assuming that signal contains uncorrelated noise)

   # Creating the inverse white noise covariance operator
   inv_cov = brahmap.InvNoiseCovLO_Diagonal(
       size=nsamples,      # Size of the inverse noise covariance operator
   
       input=[...],        # Noise covariance (variance for stationary white 
                           # noise) array
   
       dtype=np.float64,   # Numerical precision of the operator
   )
   
   # Pre-processing the pointing information
   processed_samples = brahmap.ProcessTimeSamples(
       npix=npix,                  # Number of pixels on which the map-making 
                                   # has to be done
   
       pointings=pointings,        # A 1-d of pointing indices
   
       pol_angles=pol_angles,      # A 1-d array containing the polarization angles
                                   # of the detectors
   
       noise_weights=inv_cov.diag, # A 1-d array of noise weights, or the diagonal
                                   # elements of the inverse noise covariance matrix
   
       dtype_float=numpy.float64,  # Numerical precision to be used throughout the
                                   # map-making
   )
   

2. Creating linear operators

   # Pointing operator
   pointing_LO = brahmap.PointingLO(processed_samples)
   
   # Block-diagonal preconditioner
   precond_LO = brahmap.BlockDiagonalPreconditionerLO(processed_samples)
   

3. Performing the map-making (GLS in this example)

   A = pointing_LO.T * inv_cov * pointing_LO
   b = pointing_LO.T * inv_cov * tod_array
   
   # Solving for x in the linear equation A.x=b using preconditioner
   map_vector = scipy.sparse.linalg.cg(A, b, M=precond_LO)
   

4. Post-processing to produce the sky maps. Note that map_vector from previous step contains maps in the form \([I_1, Q_1, U_1, I_2, Q_2, U_2, \dots]\). This has to be separated into I, Q, and U maps while taking care of the unobserved (masked) pixels.

   # Separate I, Q, and U maps
   output_maps = separate_map_vectors(map_vector, processed_samples)
   
   # output_maps[0] --> I map
   # output_maps[1] --> Q map
   # output_maps[2] --> U map
   

GLS map-making

BrahMap provides a simple wrapper function for GLS map-making as well:

# Creating the inverse white noise covariance operator
inv_cov = brahmap.InvNoiseCovLO_Diagonal(
    size=nsamples,      # Size of the inverse noise covariance operator

    input=[...],        # Noise covariance (variance for stationary white 
                        # noise) array

    dtype=np.float64,   # Numerical precision of the operator
)

# Performing the GLS map-making
gls_result = brahmap.compute_GLS_maps(
    npix=npix,                      # Number of pixels on which the map-making
                                    # has to be done

    pointings=pointings,            # A 1-d of pointing indices

    time_ordered_data=tod_array,    # A 1-d array of time-ordered-data

    pol_angles=pol_angles,          # A 1-d array containing the polarization angles
                                    # of the detectors

    inv_noise_cov_operator=inv_cov, # Inverse noise covariance operator

    dtype_float=np.float64,         # Numerical precision to be used in map-making
)

gls_result obtained above is an instance of the class GLSResult. The output maps can be accessed from this object with gls_result.GLS_maps.

GLS map-making with litebird_sim data

BrahMap is also integrated with the LiteBIRD simulation framework litebird_sim. It provides a wrapper function for GLS map-making that uses a list of Observation instances and a suitable inverse noise covariance operator to produce the sky maps.

The MPI communicator used in map-making must be the one that contains exclusively all the data needed for map-making. In case of litebird_sim, the communicator lbs.MPI_COMM_GRID.COMM_OBS_GRID is a subset of lbs.MPI_COMM_WORLD, and it excludes the MPI processes that do not contain any detectors (and TODs). Therefore, it is a suitable communicator to be used in map-making. Therefore, communicator used by BrahMap must be updated as following before using any other BrahMap function with litebird_sim data: brahmap.MPI_UTILS.update_communicator(comm=lbs.MPI_COMM_GRID.COMM_OBS_GRID)

# Creating the inverse white noise covariance operator
inv_cov = brahmap.InvNoiseCovLO_Diagonal(
    size=nsamples,      # Size of the inverse noise covariance operator

    input=[...],        # Noise covariance (variance for stationary white 
                        # noise) array

    dtype=np.float64,   # Numerical precision of the operator
)

# Performing the GLS map-making
gls_result = brahmap.LBSim_compute_GLS_maps(
    nside=nside,                    # Nside parameter for the output healpix map
    observations=sim.observations,  # List of observations from litebird_sim
    components="tod",                # TOD component to be used in map-making
    inv_noise_cov_operator=inv_cov, # Inverse noise covariance operator
    dtype_float=np.float64,         # Numerical precision to be used in map-making
)

gls_result obtained above is an instance of the class LBSimGLSResult. The output maps can be accessed from this object with gls_result.GLS_maps.