To perform multiple observations to a high standard and obtain several images of open clusters for analysis.
Working with Paul Hallam and Ryan Cheale, compare dark frames for a variety of temperatures and exposure lengths and confirm that they do not vary with time.
Use python to write a program to analyse the dark frames and produce histograms and axis projections.
Write a program to simulate a star field.
Write a program to count the number of stars in an open cluster.