Slitless spectroscopy
Slitless spectroscopy is astronomical spectroscopy done without a small slit to allow only light from a small region to be diffracted. It works best in sparsely populated fields, as it spreads each point source out into its spectrum, and crowded fields will be too confused to be useful. It also faces the problem that for extended sources, nearby emission lines will overlap.
The Crossley telescope utilized a slitless spectrograph that was originally employed by Nicholas Mayall.[1]
Florence Cushman employed this method at the Harvard College Observatory to classify hundreds of thousands of stars in the Henry Draper Catalogue.[2]
References
- ^ Wilson 2004, p. 432
- ^ "Florence Cushman", Wikipedia, 2020-02-12, retrieved 2020-05-02
Cited sources
- Wilson, Ray N. (2004), Reflecting Telescope Optics, Volume 1: Basic design theory and its historical development, Astronomy and astrophysics library, vol. 1, Springer, ISBN 978-3-540-40106-3
See also
 | This astronomy-related article is a stub. You can help Wikipedia by expanding it. |