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Phil Marshall edited this page Mar 22, 2013
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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)