This paper presents an introduction on the use of the Python language for astronomy and spectroscopy to perform rapid spectrum analysis of the gam Cas star. … Continue readingPython for astronomy and spectroscopy : Rapid spectrum analysis
An important step in the processing of raw data in spectroscopy is wavelength calibration. The SCCN model, allows to assist the astronomer in this step with an AI … Continue readingSCCN Model : Spectral Calibration by Artificial Intelligence
The Python-based application FitsViewerLight is a FITS file viewer that can display both raw images and spectra. … Continue readingFITS Light Python Viewer
SpecBok is a Python script using the Bokeh library in order to generate Interactive Web Spectra from FITS files. … Continue readingSpecBok : Spectra Generator for the web in Python
Within the astronomy observatories there are so-called “Observatory Log Books”. These notebooks are used to record all the important informations concerning the observation sessions carried out by the astronomer with the telescope.
Because i have to start with something, for my first spectrum i chose a very bright star, Vega (Alpha Lyrae), the brightest star in the Lyra constellation.