269001 VO Computational Concepts in Astronomy and Geosciences I (2021W)
Labels
REMOTE
Registration/Deregistration
Note: The time of your registration within the registration period has no effect on the allocation of places (no first come, first served).
Details
Language: English
Examination dates
- Tuesday 25.01.2022 09:45 - 11:15 Digital
- Tuesday 01.03.2022 09:45 - 11:15 Digital
- Tuesday 10.05.2022 09:45 - 11:15 Digital
- Tuesday 05.07.2022 09:45 - 11:15 Digital
Lecturers
Classes (iCal) - next class is marked with N
Lectures will be held online.
- Tuesday 12.10. 09:45 - 11:15 Digital
- Tuesday 19.10. 09:45 - 11:15 Digital
- Tuesday 09.11. 09:45 - 11:15 Digital
- Tuesday 16.11. 09:45 - 11:15 Digital
- Tuesday 23.11. 09:45 - 11:15 Digital
- Tuesday 30.11. 09:45 - 11:15 Digital
- Tuesday 07.12. 09:45 - 11:15 Digital
- Tuesday 14.12. 09:45 - 11:15 Digital
- Tuesday 11.01. 09:45 - 11:15 Digital
- Tuesday 18.01. 09:45 - 11:15 Digital
Information
Aims, contents and method of the course
The aim of this course is to introduce students to a range of computational concepts useful in astronomy and geosciences. The course is split into the following topics:1) Data processing in space instrumentation: Students will gain insight into software dealing with space instrumentation. The lectures explain what software tasks are carried out on board of space telescopes, what algorithms are being used e.g. for data compression and what the challenges in their implementation are. In this context software engineering and quality assurance are also briefly touched.2) Statistics: students will learn about probabilistic programming languages (PPLs) with the aim of being able to apply these to their data modelling problems. PPLs are modern computational tools for statistical inference. The course will give some background in probabilistic models and discuss various inference methods (e.g. variational inference and varieties of MCMC sampling) and their pros/cons. We will then introduce PPLs with several worked examples on data-modelling problems.3) Dynamics of stellar galactic and gaseous protoplanetary disks: Students will be introduced to the concept of hydrodynamics, which is ubiquitously used in astronomy, in particular, to describe the evolution of galaxies and protoplanetary disks around young stars. Numerical methods to compute the gravity force of astrophysical objects and the friction force between gas and dust grains in protoplanetary disks will be presented.
Assessment and permitted materials
Written exam at the end of the semester
Minimum requirements and assessment criteria
more than 50% at the written exam
Examination topics
Lecture materials (slides, Jupyter Notebooks) and additional information during the lectures
Reading list
see lecture
Association in the course directory
CO-AST1
Last modified: Sa 08.07.2023 00:21