Spectrograph Red Leak Test

Details Spectrograph Red Leak Test Spectrograph Red Leak Test

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.1343c&link_type=abstract

HST Proposal ID #1343

Physics

Hst Proposal Id #1343 Solar System

Scientific paper

This test features the measurement of one star, 16 Cyg B = HD 186427, with both spectrographs, in the range 1530-3230A. The goal of the test is to achieve S/N = 35 to 50A at 5A resolution. The star is an HST ultraviolet standard, and it is also a near-solar analog. The purpose of the test is to measure the amount of red leak into the ultraviolet region for an object with a color that is very similar to solar system objects. The information is necessary for efficient planning.

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