view Abstract Citations (2) References Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Performance of Multistage Image Amplifying Tubes; Astronomical Applications; and Proposed Use with Fabry-Perot Etalons for Stellar Spectroscopy. Dunham, T., Jr. Abstract and Weekly, B., Nature 185, 370, 1960) offer advantages for photometry at low flux levels: (1) high- speed recording; (2) background electrons are focused at the output, thereby reducing the number per resolution band to approximately 10-~ of the contribution encountered with photomultipliers; and (3) scintillations, corresponding to individual photoelectrons, are bright enough to permit recording a considerable fraction on moving film. Information storage is greater on moving film and scintillations in individual spectral resolution bands can be counted, so that the tubes can be used as multi- channel pulse counters [Dunham, T., Jr., J. Opt. Soc. Am. 50, 1129(A), 19601. The factor of merit of an image tube for spectrophotometry may be expressed as G2r2/N, where G is the over-all light gain, r the linear resolution, and N the background. For direct stellar photometry, an image tube offers the possibility of recording flux from a number of star images (and sky) simultaneously, using fiber light guides to transfer images to a linear array on the photocathode, so that scintillations can be recorded and counted on moving film. Speed, resolution, and background have been investigated, using test spectra and coude' spectra with Baum's microprojector (Baum, W. A., Advances in Electronics and Electron. Phys. 16, 391, 1962). The percentage of incident photons that can be recorded on film has been determined by using a low-intensity scattering source of approximately monochromatic light. For high-resolution spectroscopy, the use of an image tube and moving film, with a scanning FabryPerot etalon (Jacquinot, P., and Dufour, C., J. Reck., Cent. Nat. Rech. Sci. 2, 19,1948) and rotating grating, appears to offer an efficient system that permits pulse counting of many fringes simultaneously. For space spectroscopy, direct electrical pickup at the output, on narrow conducting strips corresponding to the fringes, and connected to individual pulsecounting circuits, would have advantages. The experimental part of this study was carried out at Imperial College, thanks to the kindness of Dr. J. D. McGee. Publication: The Astronomical Journal Pub Date: June 1962 DOI: 10.1086/108872 Bibcode: 1962AJ.....67R.575D full text sources ADS |
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