Slitless Spectroscopy
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Slitless spectroscopy is astronomical
spectroscopy Spectroscopy is the field of study that measures and interprets the electromagnetic spectra that result from the interaction between electromagnetic radiation and matter as a function of the wavelength or frequency of the radiation. Matter ...
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. The Henry Draper Catalogue, published 1924, contains stellar classifications for hundreds of thousands of stars, based on spectra taken with the objective prism method at
Harvard College Observatory The Harvard College Observatory (HCO) is an institution managing a complex of buildings and multiple instruments used for astronomical research by the Harvard University Department of Astronomy. It is located in Cambridge, Massachusetts, United S ...
. The work of classification was led initially by Williamina Fleming and later by
Annie Jump Cannon Annie Jump Cannon (; December 11, 1863 – April 13, 1941) was an American astronomer whose cataloging work was instrumental in the development of contemporary stellar classification. With Edward C. Pickering, she is credited with the creation of ...
, with contributions from many other female astronomers including Florence Cushman.


See also

* Fine Guidance Sensor and Near Infrared Imager and Slitless Spectrograph (JWST component) * Echelle grating


References


Cited sources

* * Astronomical spectroscopy {{spectroscopy-stub