Redshifts of a BSO and galaxies in the vicinity of the radio source RN 8.
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Engineering topics
Publications and source records attributed to Wampler, E. J..
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The papers presented at the symposium are given which deal with the present state of sensors, as may be applicable to the Large Space Telescope (LST) program. Several aspects of sensors are covered including a discussion of the properties of photocathodes and the operational imaging camera tubes.
Determination of redshifts for two galaxies in the group associated with the quasi-stellar source PKS 2251 + 11 from the measurements of the H and K absorption lines of Ca II. The measured redshift of the brighter galaxy is within 60 km/sec of the redshift of the quasi-stellar source. The other differs by 1000 km/sec. Strong hydrogen-line emission reported earlier for the brighter galaxy was not detected.
A scanner that uses an image dissector to scan the output screen of an image tube has proven to be a sensitive and linear detector for faint astronomical spectra. The image-tube phosphor screen acts as a short-term storage element and allows the system to approach the performance of an ideal multichannel photon counter. Pulses resulting from individual photons, emitted from the output phosphor and detected by the image dissector, trigger an amplifier-discriminator and are counted in a 24-bit, 4096-word circulating memory. Aspects of system performance are discussed, giving attention to linearity, dynamic range, sensitivity, stability, and scattered light properties.
Description and evaluation of the remotely operated Lick Observatory Cassegrain focus of the 120-inch telescope. The experience with this instrument has revealed that an automated system can profoundly change the observer's approach to his work. This makes it difficult to evaluate the 'advantage' of an automated telescope over a conventional instrument. Some of the problems arising with automation in astronomy are discussed.
Nuclei reddening of Seyfert galaxies NGC 1068 and 1275 from photoelectric spectrophotometric observations
Phosphor-output image intensifier response to single photon inputs in multichannel spectrophotometer for faint optical sources
Lunar laser beam retroreflection observations, showing agreement with predicted ephemeris and signal strength
Optical observations of pulsar NP 0532, comparing light curves in IR and UV, noting polarization
Crab Nebula pulsar NP 0532 simultaneous optical and radio observations, noting influence of interstellar dispersion value uncertainty
Crab Nebula pulsar detection by TV camera with image intensifier at focus of astronomical telescope, detailing instrumentation and observations
IR and violet sulfur lines for Seyfert galaxies, noting substantial reddening in nuclei
Photoelectric scanner observations of various quasi-stellar objects, discussing line intensities
Photoelectric spectrophotometric study of emission line spectrum of quasi-stellar source
Hydrogen emission lines photoelectric measures in Ton 1542 indicates radiative recombination in upper levels and sharp intensity increase in red ascribed to nonthermal sources
Spectral energy distribution of source 3C 446 between August 17 and December 12, 1966
Radio telescope-spectrophotometric scanner investigation of continuous energy distribution of four quasars