Astrophysical Data Analyses
Overall Course Objectives
Based on hands-on activities, the course gives the participants a working knowledge of astronomical data acquisition, analysis, and scientific exploitation. The course trains students in using professional software and tools to analyze real astronomical data from a series of different wavelengths and telescopes.
See course description in Danish
Learning Objectives
- use a computer with the Linux command line system and shell-scripts
- search through scientific databases and archives for specific instrument data
- perform scientific analysis of astronomical data across the electromagnetic spectrum
- reduce X-ray, optical, millimeter wavelength and radio data
- examine astrophysical data with dedicated methods and tools
- assess data quality from a statistical perspective
- exploit observation products such as images, light-curves, and spectra
- utilize fitting techniques to apply a model or mathematical function to data
- solve real astrophysical problems and tailored exercises
- interpret, evaluate and describe the results.
Course Content
The course starts with an introduction to the use of the Linux command-line system (incl. scripts), followed by basic knowledge about astronomical detectors, calibration, measurement significance, and noise sources. The participants are trained in reducing imaging and spectroscopic data and performing photometry. The students learn about single-dish and interferometric observations at millimetres and radio wavelengths and get to reduce and analyze continuum and spectroscopic data. X-ray data from currently flying X-ray instruments (e.g. NuSTAR, INTEGRAL, NICER) are provided and analyzed to generate scientific products (images, light curves, and spectra). All lectures are followed by hands-on exercises based on the methods and techniques described during the lectures. Example applications include analyzing the spectra of galaxies and supernova explosions, applying techniques to find exoplanets, measuring the molecular content of distant galaxies, and studying thermonuclear explosions on neutron stars.
Possible start times
- 6 – 20 (Tues 13-17)
Teaching Method
Lectures and practical exercises.
Faculty
Remarks
The course provides a good preparation to the Nordic Optical Telescope (NOT) Summer School.
Limited number of seats
Maximum: 20.
Please be aware that this course has a limited number of seats available. If there are too many applicants, a pool will be created for the remainder of the qualified applicants, and they will be selected at random. You will be informed 8 days before the start of the course, whether you have been allocated a spot.




