Metallicity
In this exercise you will be given a large data set and plot
it in such a way that meaningful conclusions can be reached in regards
to the metalicity profile of our galaxy. Metalicity is one of the nine
dimensions that will eventually make up our map of the Milky Way
galaxy. Metalicity is the ratio of heavy elements present in a
star to lighter elements such Hydrogen, Helium, or Lithium. What we
will be using in this exercise is the ratio of Iron to Hydrogen (Fe/H).
Metalicity can be treated as an analog to the age of the star,
basically the higher the metalicity the younger the star, and
vice-versa . If you are interested in learning more about why this is
feel free to read this
introductory article.
The first requirement is that you possess R, a free data manipulation program. Links to download it can be found in the useful program downloads page. Once you have downloaded and installed R it is highly advised that you read through the short tutorial explaining some basic principals and commands.