Abstract
AbstractA method for a fully automatic reduction of digitised objective prism spectra is developed. It leads to positions and radial velocities, magnitudes and intensities of spectral lines. The latter then can be used for classification purposes. The system is tested with plates taken with a specific telescope-prism-filter combination.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
