6 EC
Semester 1, period 1, 2, 3
5092ASOL6Y
During this practicum the students will obtain spectroscopic data using the telescopes and instrumentation of the Anton Pannekoek Observatorium. The students will get familiar with the techniques and methods and will understand the importance of spectroscopy for astronomy and astrophysics. The students will choice a target (from a list of targets) and they will write a proposal to observe this target to obtain the desired (astro-)physical information from it. The proposal will be evaluated and graded by their fellow students using a peer review system. The students will perform their proposed observations themselves (under guidance of a teaching assistant) using the available telescopes and spectrographs of the observatory. After the observations have been completed successfully, the students will reduce and analyze the obtained data themselves using the available software packages. The students will present their results during a presentation in front of the class, in which they also will interpret the results and draw conclusions about the scientific questions they wanted to address with their observations.
Manuals on how to observe with the difference instruments
Data analysis software; partly in Python
College slides via Canvas. Additional literature (also via Canvas).
- The lectures are needed to learn the basic concepts of spectroscopy, observing, and planning observations. The students are expected to attend the lectures, watch and study the associated online video's, and to perform self study with the given lecture notes.
- Using a practice observing run during daytime (of the day time sky, either blue or cloudy sky) the students will take observations using the same instruments as during the night time. With this observations the students will practice taken data and reducting and analysing the obtained data so that they are well prepared for the night time observation run. The daytime observations are performed betweein mid-September and mid-October.
- The night observations will start around mid-October and can last until Christmas. The students will observe in groups of 3 to 4 students and will be assisted by a teaching assistant (TA) throughout the night. After the basic introduction by the TAs in combination with the obtained experience during the daytime observing run, the students are expected to perform the observations mostly by themselves with only the basic guidance by the TAs. The TAs will judge the quality of the observing the students performed (as well as the data reduction and analysis, see next point).
- After the observations, the students (with basic help and input of the TAs) will reduce, analyze and interpret their obtained data so that at the end of block 3 the students can present their results during a presentation in front of all students. Mostly this work will be done by the students themselves. The presentation will be judge by the lecturer and the TAs.
|
Activity |
total hours |
|
Lectures and homework |
40 |
|
Project based work |
128 |
Programme's requirements concerning attendance (TER-B):
Additional requirements for this course:
| Item and weight | Details |
|
Final grade |
Contact the course coordinator to make an appointment for inspection.
Homework and observing log - 30%
Presentation and discussion in december (group grade) - 40%
Final presentation (group grade) - 30%
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
The course structure will be shared with the students on the first lecture.
Recommended prior knowledge: Elementary knowledge of Optics, and first and second year astrophysics and physics courses.
Max. participants: 20 students. Students work in groups of typically 3 students.
Technical support