Supplementary material for PRD 89, 042001 (arXiv:1310.0828)
Contact: Alex Drlica-Wagner <kadrlica@fnal.gov>

This distribution contains machine-readable
text files corresponding to the analysis and 
results of PRD 89, 042001. These files can be divided
into three categories:

===============================
=== Dark Matter Constraints ===
===============================
Number of files: 6
File naming: limits_<channel>.txt
Reference: Table II - Table VII
Description:
    Machine-readable version of Table II - Table VII
Structure:
    Column [0]:    Dark matter particle mass (GeV)
    Column [1-25]: Constraints on <sigmav> derived
        from each dwarf galaxy with a kinematically
        determined J-factor.
    Column [26]:   Constraints on <sigmav> derived
        from a combined analysis of 15 dwarf galaxies.

===========================
===  Bin-By-Bin Limits  ===
===========================
Number of files: 1
File naming: bin_by_bin_limits.txt
Reference: Figure 3
Description:
    Measured bin-by-bin upper limits for each dwarf
    spheroidal galaxy as displayed by the solid 
    black arrows in Figure 3. 
Structure:
    Column [0]:    Geometric mean of the bin energy (MeV).
    Column [1-25]: Energy flux upper limit derived from
        each dwarf galaxy in the energy bin specified by
        Column [0].

================================
===  Bin-By-Bin Likelihoods  ===
================================
Number of files: 25
File naming: like_<dwarf>.txt
Reference: Section III
Description:
    These files contain likelihood functions for each dwarf derived 
    energy-bin by energy-bin, tabulated as the delta log-like value 
    for 25 different values of the energy flux of a putative dwarf source.
Structure:
    Column [0-1]: Minimum and maximum energy edges of each
        bin.
    Column [2]:   Energy flux of a putative dwarf source
        integrated over the specified bin.
    Column [3]:   Delta log-likelihood as a function of
        the energy flux of the source

=========================
===  Example Scripts  ===
=========================
Also included in this directory are a set of example scripts to 
aid with a few potential usage cases. These scripts are merely 
meant to illustrate how to operate with the data included here 
and *DO NOT* represent a rigorous analysis, nor do they constitute 
a fully fledged interface to the data themselves. A brief 
description of the examples is included below.

example1.py -- This example demonstrates how to load 
               and plot the dark matter limit files.
example2.py -- This example demonstrates how to load
               and plot the bin-by-bin likelihood limits.
example3.py -- This example demonstrates how to load
               the bin-by-bin likelihood functions and a 
               gamma-ray spectrum and compute spectrally-
               dependent dark matter limits on the 
               annihilation cross section.
               NOTE: This script *DOES NOT* incorporate 
               uncertainties on the measured J-factor.


--- Updates --- 
02-00-01 (kadrlica, 10/30/2014): Fixed typos in the README