Mid-infrared spectrophotometry of Saturn's ring system
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spectrophotometry mid-IR Saturn's rings↗
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Infrared Spectrophotometry Of Io Between 2-13 um
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infrared spectrophotometry Io thermal emission↗
The Fourier Transform in Interferometric Spectrophotometry
Fourier transform in interferometer spectrometry measurements
SPECTROPHOTOMETER↗
Photoelectric spectrophotometry of quasi- stellar sources.
Spectral energy distributions of various quasi- stellar radio sources, using photoelectric spectrum scanner
ENERGY SPECTRUM↗
Blood oxygen saturation determined by transmission spectrophotometry of hemolyzed blood samples
Use of the Lambert-Beer Transmission Law determines blood oxygen saturation of hemolyzed blood samples. This simplified method is based on the difference in optical absorption properties of hemoglobin and oxyhemoglobin.
Malik, W. M.↗
Spectrophotometry of the sunspot observed on June 19, 1959
Physical parameters for sunspot, and graphic method of determining excitation temperature from growth curve
GROWTH↗
Rocket ultraviolet spectrophotometry in the Orion region.
Low resolution UV spectrography of several bright stars in Orion region photographed from Aerobee rocket
Boggess, A., III↗
Photoelectric spectrophotometry of quasi- stellar sources
Spectral energy distribution in quasars, using photoelectric spectral scanner in several wavelength ranges
Oke, J. B.↗
Spectrophotometry and infrared photometry of BL Lacertae.
Variable star BL Lacertae absolute spectral energy distribution in visible and IR regions, noting synchrotron features and possible quasar nature
Becklin, E. E.↗
The future of photometry and moderate resolution spectrophotometry in space astronomy
Photometric and spectrophotometric measurements in space astronomy
Code, A. D.↗
Photoelectric spectrophotometry of B264
Quasar B264 observed with multichannel spectrometer attached to 200 inch telescope, comparing to N-type and Seyfert galaxies and other quasars
Oke, J. B.↗
Photoelectric spectrophotometry of 4C 05.34
Quasar 4C 05.34 absolute spectral energy distribution by multichannel photoelectric spectrometry
Oke, J. B.↗
Spectrophotometry of comets 1967n, 1968b, and 1968c
Ikeya-Seki /1967n/, Thomas /1968b/ and Honda /1968c/ comet photoelectric spectrum, examining swan bands, continuum and reflected scattered light
Gebel, W. L.↗
Spectrophotometry of Pluto
Pluto albedo at various wavelengths from spectrophotometric measurements
Fix, J. D.↗
Photoelectric spectrophotometry of Seyfert galaxies
Nuclei reddening of Seyfert galaxies NGC 1068 and 1275 from photoelectric spectrophotometric observations
Wampler, E. J.↗
Spectrophotometry of Comet 1969g - Tago- Sato-Kosaka
Comet 1969g spectrum at 3800-8500 A, noting upper H alpha surface brightness limit consistency with chromospheric resonance fluorescence model
Odell, C. R.↗
Saturn and its satellites - Narrow-band spectrophotometry, 0.3-1.1 micron
Saturn satellites spectrophotometric observations at UV, visible and near IR, noting reflection spectra data
Elias, J. H.↗
Absolute ultraviolet spectrophotometry of: alpha CMa, gamma Ori, kappa Ori, and alpha Leo; and a continuing calibration program and some preliminary results
Spectral observations of the stars alpha CMa, gamma Ori, kappa Ori, and alpha Leo have been obtained in the range 1150 to 4000 Angstroms, using rocket borne spectrometers. The payloads have a 13-inch diameter telescope, a rotatable concave diffraction grating, and three pulse counting photomultiplier photometers. The laboratory standards used as photometric references derive their primary calibration directly or indirectly from the National Bureau of Standards. An error range of up to + or - 10 percent is attributed to these laboratory standards; + or - 8 percent to the calibration procedure; and + or - 10 percent is assigned as an accidental error range.
Evans, D. C.↗