To introduce students to the experimental techniques which enable astrophysicists to use the electromagnetic spectrum to study the physics of astronomical objects; to become familiar with the design of telescopes in the optical and infrared; to understand the physical basis of light detection in the optical; to understand observing techniques such as photometry, spectroscopy, and adaptive optics.

(LO1) Apply physical principles (such as waves, electromagnetism, thermodynamics, and quantum physics) to situations relevant to astronomical observing.

(LO2) Apply common experimental concepts (including signal-to-noise ratio, sampling, and resolution) to observational astrophysics.

(LO3) Choose the appropriate technique and experimental design to achieve a specific science goal in observational astrophysics.

(LO4) Understand how physical principles have influenced the designs of current and planned astronomical facilities.

(S1) Problem solving skills.

(S2) Applied mathematical reasoning skills.

Basic design and principles of operation of telescopes and detectors across the electromagnetic spectrum, with a focus on optical and near infrared. Photometry/imaging, spectroscopy/dispersive techniques, interferometry. Sampling, resolution, signal-to-noise ratio. Planning and interpreting observations.

Teaching Method 1 - Lecture
Attendance Recorded: Yes

Teaching Method 2 - Tutorial
Attendance Recorded: Yes

All lecture notes made available from beginning of module via VLE.

All lectures are recorded, and can be streamed by the students via the VLE within 1 day of the lecture.

All problem sets, whether formative or summative, are made available via VLE 1 week in advance of due date. Model solutions the problems are released 1 week after deadline, via VLE.