Syllabus
Methods of observations and astrophysical data reduction: Spectroscopy. Program and objectives:
1. Description of the 2-m telescope and slit spectrograph, dispersion.
2. Selection of targets according to the scientific program: emission stars, symbitic stars, spectroscopic and eclipsing binaries. Emission and absorption spectra. Balmer series.
3. Calibration frames (comparison spectrum Th-Ar, darkframe, flatfield).
4. Reduction of measured spectra, spectral line identification, radial velocities determination. Tasks are processed via remote access to the 2-m telescope or directly in the dome of AI ASCR in Ondrejov.
Annotation
Methods of observations and astrophysical data reduction: Spectroscopy.
Description of the 2-m telescope and spectrograph, selection of targets.
Emission and absorption spectra. Calibration (comparison spectrum, darkframe, flatfield). Reduction of measured spectra, spectral line identification, radial velocities determination.
Tasks are processed via remote access to the 2-m telescope or directly in the dome of AI ASCR in Ondrejov.