Paper
3 May 1979 Wide-Field Electrographic Cameras For Imagery And Spectrography At Visual And Middle-UV Wavelengths
Harry M. Heckathorn, George R. Carruthers, Seth D. Shulman
Author Affiliations +
Abstract
The use of a Kron electrographic detector for wide-field, narrow-band imagery of faint emission nebulosity in the near-UV and visual (3100-6000 A) wavelength interval is de-scribed. As an example of the photometric quality of the imagery and of the sensitivity of the instrumentation to diffuse, low-contrast objects, imagery of the Cygnus Loop super-nova remnant in the high excitation line of [Ne V]λ3426 A is presented. In addition, we describe our current program to develop electrographic detectors which use cesium tellu-ride photocathodes for broad-band imagery and spectrography in the middle-UV (1650-3100 A) wavelength range.
© (1979) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Harry M. Heckathorn, George R. Carruthers, and Seth D. Shulman "Wide-Field Electrographic Cameras For Imagery And Spectrography At Visual And Middle-UV Wavelengths", Proc. SPIE 0172, Instrumentation in Astronomy III, (3 May 1979); https://doi.org/10.1117/12.957093
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Sensors

Cameras

Astronomy

Visualization

Cesium

Image resolution

Interference filters

RELATED CONTENT

Environmental modeling using omnidirectional vision sensors
Proceedings of SPIE (November 22 1999)
General relationship for optimal tracking performance
Proceedings of SPIE (October 29 1996)
SPOT MTF Performance Evaluation
Proceedings of SPIE (November 25 1986)

Back to Top