Optimizing Results from Automatic Objective-Prism Surveys

Details Optimizing Results from Automatic Objective-Prism Surveys Optimizing Results from Automatic Objective-Prism Surveys

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.263...95g&link_type=abstract

Astrophysics and Space Science, Volume 263, Issue 1-4, pp. 95-98

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

One of the most important results in observational cosmology is the galaxy star formation rate distribution, or its equivalent observable, the Hα luminosity function. The UCM-CIDA project has grown to address the problem of the poorly-known faint star forming galaxy population using the objective-prism technique along with a CCD mosaic in a Schmidt telescope.

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