450101 SE DYNamics Age and Metallicity Indicators Tracing Evolution (PI) (2020W)
Continuous assessment of course work
Labels
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).
- Registration is open from Th 10.09.2020 10:00 to Mo 28.09.2020 23:59
- Registration is open from Th 01.10.2020 10:00 to Tu 13.10.2020 23:59
- Deregistration possible until Tu 13.10.2020 23:59
Details
max. 15 participants
Language: German, English
Lecturers
Classes (iCal) - next class is marked with N
Thursday
01.10.
13:15 - 14:45
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday
08.10.
13:15 - 14:45
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday
15.10.
13:15 - 14:45
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday
22.10.
13:15 - 14:45
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday
29.10.
13:15 - 14:45
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday
05.11.
13:15 - 14:45
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday
12.11.
13:15 - 14:45
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday
19.11.
13:15 - 14:45
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday
26.11.
13:15 - 14:45
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday
03.12.
13:15 - 14:45
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday
10.12.
13:15 - 14:45
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday
17.12.
13:15 - 14:45
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday
07.01.
13:15 - 14:45
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday
14.01.
13:15 - 14:45
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday
21.01.
13:15 - 14:45
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Thursday
28.01.
13:15 - 14:45
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Information
Aims, contents and method of the course
This seminar encompasses the weekly meeting of the members of the "Dynamics of Stellar Systems" research group at the Department of Astrophysics and eternal collaborators, who are involved in developing the DYNAMITE (DYNamics Age and Metallicity Indicators Tracing Evolution) code.The DYNAMITE code is a synergy and extension of our existing Schwarzschild orbit-superposition and discrete chemo-dynamical numerical implementations. By fitting simultaneously the extracted stellar motions and population properties, the aim is to uncover the luminous and dark matter distribution of these galaxies as well as to unravel their formation history.Participants discuss and present the step-wise implementation, testing and applications of the DYNAMITE code.
Assessment and permitted materials
The assessment will be based on active participation, i.e., contributing to the discussions through asking questions and providing input.
Minimum requirements and assessment criteria
The meetings are in English. Given the specialised nature of the meetings, a background in stellar dynamics as well as proficient C(++) and/or Python coding skills are required. A minimum participation of 75% is required as well as at least one informal presentation.
Examination topics
Topics related to the DYNAMITE code.
Reading list
Potential reading materials will be suggested in the meeting announcements.
Association in the course directory
Last modified: Th 01.10.2020 09:11