This python package explores how the measured rotation curve of the Milky Way galaxy constrains the dark matter density distribution in our galaxy. Of particular interest are the variations in the dark matter density at the location of the earth.

For: Data Analysis (PHYS 201), Spring 2017, Harvard University. Create by: Daniya Seitova, Jun Yin License:GNU General Public License v3

Package Manual:

model.ipynb : shows the contents where we import our package, load our test data, do some inference using our model, and show some plots.

msdmd/testdmdcode.py : test the code

nsdmd/model.py : the module for our model

nsdmd/io.py : the module containing functions for loading data files

nsdmd/data/ : directory containing example and reference data files