The main aims of this project are to observe a star to obtain its spectrum, then analyse this to find its composition and which line broadening methods are dominant in the star.
A link to the logbook for calibration, observation and meeting can be found here:
https://twiki.ph.rhul.ac.uk/twiki/bin/view/Public/StewartBoogertSpectroscopy2015
-- JosephBayley - 16 Nov 2015