Accession Number : AD0785137
Title : The Limits of Detectability of a Low-Light-Level Point-Source Sensor as a Function of Telescope Aperture, Sensor Resolution, Night-Sky Background, and Pre-readout Electron Gain.
Descriptive Note : Technical note,
Corporate Author : MASSACHUSETTS INST OF TECH LEXINGTON LINCOLN LAB
Personal Author(s) : Weber,Robert ; Brooks,Thomas H.
Report Date : 16 AUG 1974
Pagination or Media Count : 127
Abstract : Based on laboratory measurements and on field experience in detecting G-type stars and point-objects by reflected sunlight, a figure of performance of a low-light-level sensor operating continuously at standard TV rates and incorporating a variable pre-readout current gain of 20,000 has been developed and extrapolated to specify limiting detectable point-source visual magnitudes for telescope apertures ranging from 7 in. to 400 in., and for image-cell angular diameters from 0.5 to 60.0 sec. The detection criterion, expressed in video SNR, is that the point-source images in typical real-sky situations be detectable on the screen of a video monitor (with essentially 100% probability of detection) by a human observer. After three limiting cases are discussed, camera-tube saturation is considered. Levels are determined for the present sensor and for sensors of the future. (Modified author abstract)
Descriptors : *OPTICAL DETECTORS, *TELESCOPES, LOW LIGHT LEVELS, ELECTROOPTICS, SOURCES, TELEVISION SYSTEMS
Subject Categories : Astronomy
Distribution Statement : APPROVED FOR PUBLIC RELEASE