Becoming familiar with astrophysics concepts used in later modules
Taking reliable and reproducible data
Developing an understanding of various techniques of data gathering and analysis in modern astrophysics
Calculating experimental results and their associated uncertainties
Using computer software, including specific astrophysical software, to analyse data
Writing a coherent account of the experimental procedure and conclusions
Understanding physics in depth by performing specific experiments
Developing practical, technical and computing skills required for later modules

(LO1) Improved practical skills and experience.

(LO2) A detailed understanding of the fundamental physics and/or astrophysics behind the experiments.

(LO3) Familiarity with IT package for calculating, displaying and presenting results

(LO4) Familiarity with subject specific astrophysics data analysis software.

(LO5) Enhanced ability to plan, execute and report the results of an investigation.

(LO6) Knowledge of the methods employed in the detection and analysis of light at optical wavelengths from astrophysical sources

(LO7) A clear understanding of the methods employed in astronomical photometry and spectroscopy.

(LO8) Understanding of the acquisition, reduction and analysis of astronomical data.

(LO9) Experience of the acquisition, reduction and analysis of astronomical data.

(S1) Numeracy/computational skills - Confidence/competence in measuring and using numbers

(S2) Critical thinking and problem solving - Critical analysis

(S3) Critical thinking and problem solving - Evaluation

1

The laboratory-based section of the module will consist of practical experiments around the analysis of optical frequency light in astronomy, for example:

Pre-processing astronomical imaging and spectroscopic data.
The photometric and spectroscopic analysis of data.
Astrophysical distance determination.
Building and interpreting lightcurves of astronomical objects.
Interpretation of spectra of novae.

2

The lecture component will concentrate on positional astronomy and astronomical photometry, including the following areas:

Signal to noise calculations.
Detectors.
Filter systems.
Relative and absolute photometry.
Atmospheric effects.
Photometric standards.
Coordinate transformations.

The lectures will be complemented by a number of problem classes, which will be used to complete problems based on the lecture topics. A number of these problems and a final timed exercise will count towards the asses sment

Teaching Method 1 - Lecture
Description: Lectures to provide background about the practicalities of taking optical astronomical observations

Teaching Method 2 - Laboratory Work
Description: Lab based sessions to explore the technicalities of astronomical data collection and analysis

Teaching Method 3 - Other
Description: Problem classes to aid with assed worksheets set in the lectures