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Phil Marshall edited this page Mar 22, 2013 · 1 revision
NAME
    Reconstruct.py

PURPOSE
    Read in a lightcone (or list of lightcones) and compute all 
    quantities needed to estimate kappah, the convergence due to
    halos, at the centre of the lightcone. Output is a list of sample
    kappah values drawn from Pr(kappah|D), where D refers to either 
    observed data, or simulated data from a calibration line of
    sight.

COMMENTS
    The config file contains the list of lightcones to be
    reconstructed, in the form of either a directory or a single
    instance. If a directory is specified, one also gives a number
    ("batchsize") of lightcones to be reconstructed at a time. 
    The number of kappah samples desired must also be given in the
    config file.

FLAGS
    -h            Print this message [0]

INPUTS
    configfile    Plain text file containing Pangloss configuration

OUTPUTS
    stdout        Useful information
    samples       Catalog(s) of samples from Pr(kappah|D)


EXAMPLE

    Reconstruct.py example.config

BUGS

AUTHORS
  This file is part of the Pangloss project, distributed under the
  GPL v2, by Tom Collett (IoA) and  Phil Marshall (Oxford). 
  Please cite: Collett et al 2013, arxiv/###

HISTORY
  2013-03-21 started Collett & Marshall (Oxford)