6 EC
Semester 2, period 5
5214RAAS6Y
Radio astronomy opened our first window on the Universe outside the optical spectrum. It continues to play a unique role in modern astrophysics, by providing a powerful probe of primarily non-thermal emission processes important for understanding many types of astronomical objects. This emission can arise in some of the most extreme astrophysical environments, including around neutron stars and black holes. There thus exists a strong link between radio astronomy and high-energy X-ray/gamma-ray astrophysics, at the opposite end of the electromagnetic spectrum. Through the 21-cm line of hydrogen, radio astronomy is critical for mapping Galactic struture and gas content in a way inaccessible at other wavelengths.
This course gives a broad overview of the science of radio astronomy, through its relevant emission mechanisms and source classes (e.g. active galactic nuclei, HI clouds, supernova remnants, pulsars, the Sun and planets). We also provide a broad overview of the observational and analytical techniques by discussing how radio telescopes work, and how data can be analyzed to produce images of the sky. This is achieved through a series of lectures, practical work with real data, and a project in which the student writes and presents their own observing proposal - thereby gaining a deeper knowledge of a certain radio astronomical instrument and science topic.
Jupyter Notebooks
Lectures will provide the scientific content and background required for application to the various projects. The field trip to ASTRON and the Dutch radio telescopes will provide direct experience of different radio telescopes and how they are operated.
The Computer Lab Sessions using Jupyter Notebooks will teach how to handle radio astronomical data and lead to the students gaining deeper understanding of the material applied to key problems.
The students will work independently in self study time to write an observing proposal for a radio telescope and science case of their choice. This is the key assessed output of the course and will enable them to apply all the knowledge and experience gained from the other components to create their own proposal.
|
Activity |
Hours |
|
|
Excursie |
8 |
|
|
Hoorcollege |
20 |
|
|
Laptopcollege |
20 |
|
|
Presentatie |
4 |
|
|
Self study |
116 |
|
|
Total |
168 |
(6 EC x 28 uur) |
Requirements concerning attendance (OER-B).
Additional requirements for this course:
| Item and weight | Details |
|
Final grade | |
|
0.2 (19%) Pulsar practicum | |
|
0.2 (19%) Interferometer practicum | Mandatory |
|
0.2 (19%) Presentation | Mandatory |
|
0.4 (38%) Proposal final version | Mandatory |
|
0.05 (5%) Bonus FRB practicum | Best of |
1. Pulsar and Interferometry Practicums.
To be completed individually using Jupyter Notebooks
Will be graded by the TA and feedback will be provided by the TA
2. Proposal
There are two parts, the presentation and the written proposal
To be completed individually
Both parts will be graded out of 10.
Verbal feedback will be given after the presentation
Written feedback will be given on the written proposal
The 'Regulations governing fraud and plagiarism for UvA students' applies to this course. This will be monitored carefully. Upon suspicion of fraud or plagiarism the Examinations Board of the programme will be informed. For the 'Regulations governing fraud and plagiarism for UvA students' see: www.student.uva.nl
| Week number | Topics | Study Material to be prepared | Assignment Deadlines |
| 1 |
Lectures:
Practicum:
|
||
| 2 |
Lectures:
Practica:
|
Ideas for observing proposal | |
| 3 |
Lectures:
Practica:
|
Draft observing proposal | |
| 4 |
Lectures:
Practica:
|
|
|
| 5 |
Lectures:
Practica:
|
Draft observing proposal |
|
| 6 |
Practica:
|
Draft observing proposal |
|
| 7 | Excursion to ASTRON and the Dutch Radio Telescopes | ||
| 8 | Observing proposal presentations |
|
Recommended prior knowledge: a basic understanding of the Linux operating system and scripting using the python language are needed for the practicals.