Filter photometry of Saturn in the spectral region lambda lambda 2950-2450.
Rocket-borne photoelectric photometers for UV observations of Saturn, using interference filters
Bless, R. C.↗
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An analysis of Martian photometry and polarimetry.
Photometric and polarimetric properties of Mars, discussing powder covering, chemical composition and particle size of bright and dark areas and blue haze
Pollack, 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.↗
Infrared photometry of a helium star, HD 30353.
HD 30353 He binary star invisible component suggested as KO type supergiant from IR photometric data
Lee, T. A.↗
Tentative photometry of Jupiter's atmospheric activity
Photometric observation of periodic activity cycles in Jupiter atmosphere
Aksenov, A. N.↗
The future of photometry and moderate resolution spectrophotometry in space astronomy
Photometric and spectrophotometric measurements in space astronomy
Code, A. D.↗
Photometry and polarimetry of the lunar regolith as measured by Surveyor
Lunar soil and rocks photometric and polarimetric properties from high resolution Surveyor pictures
Holt, H. E.↗
X-ray photometry of M1
M1 X ray emission, examining energy interval and power law spectral distribution
Acton, L. W.↗
Multicolor photometry of supergiants and Cepheids
Color indices for stellar spectrophotometry of Cepheid variable and supergiant stars
Kelsall, T.↗
Photometry of the outer solar corona from lunar based observations
Two-dimensional isophotes of outer solar corona derived from integrated vidicon pictures taken from lunar surface by Surveyors 6 and 7
Bohlin, J. D.↗
Infrared photometry of Saturn, Titan, and the rings
Saturn, Titan and ring IR photometric observations, examining brightness temperature albedos, optical thickness and individual particles
Allen, D. A.↗
Galilean satellites - Narrowband photometry 0.30 to 1.10 microns
Jupiter Galilean satellites narrowband photometric data, observing albedos, spectral reflectivity, rotational phase, and brightness variations
Johnson, T. V.↗
A method of differential field photometry by video-photographic image subtraction
Doppler velocity field recording method over two dimensional solar active region image, using narrow band filter with video photographic subtraction technique
Fisher, R. R.↗
Mars - Narrow-band photometry, from 0.3 to 2.5 microns, of surface regions during the 1969 apparition
Mars surface narrow-band spectrophotometric observation, obtaining spectral reflectivities for geometric albedos calculation
Mccord, T. B.↗
Photometry of the outer solar corona from lunar-based observations
Two dimensional isophotes of extreme solar corona from integrated vidicon pictures taken from moon surface by Surveyors 6 and 7
Bohlin, J. D.↗
Ultraviolet photometry of the eclipsing variable CW Cephei
A series of photometric observations was made of the eclipsing variable CW Cephei on the OAO 2. Approximate elements were derived from the eclipse depths and shape of the secondary. Persistent asymmetries and anomalous light variations, larger than the expected experimental error, were also found, subsequent ground-based observations show H alpha entirely in emission, indicating the presence of an extended gaseous system surrounding one or both components. A detailed comparison was made of the flux distribution of the binary relative to that for the nominally unreddened stars delta Pic, BlIII, and eta Aur, B3V, to investigate the effects of interstellar extinction. The resultant extinction curves, normalized at a wavelength of 3330 A, show a relatively smooth increase with decreasing wavelength.
Sobieski, S.↗
Ultraviolet photometry of the moon with the celescope experiment on the OAO-2
Thirteen television frames of the moon taken in the wavelength regions of 1350-2150 A by filter U sub 3 and 1050-2150 A by filter U sub 4 in the celescope experiment are discussed. The data include phase angles from -81 deg to -26 deg. The brightness dependence on phase angle differs slightly from that of visual observations. The brightness dependence on selenographical longitude is compared with the theoretical photometric function derived by Hapke.
Ahmad, I. A.↗
Ultraviolet photometry of the eclipsing variable CW Cephei
An extended series of photometric observations were made of the eclipsing variable CW Cephei using the Wisconsin instrument on OAO-2. Approximate elements which were derived based solely on the eclipse depths and shape of the secondary are in satisfactory agreement with those found using ground based observations. However, persistent asymmetries and anomalous light variations, all larger than the expected experimental error, were also found; subsequent ground-based observations show H sub alpha entirely in emission indicating the presence of an extended gaseous system surrounding one or both of the components. Consistent solutions utilizing all data at all wavelengths were not found.
Sobieski, S.↗