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  • Other Sources  (37)
  • 1
    Publication Date: 2005-11-27
    Description: Photometric and spectrophotometric measurements in space astronomy
    Keywords: SPACE SCIENCES
    Type: NASA, WASHINGTON OPT. TELESCOPE TECHNOL. 1970; P 13-15
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  • 2
    Publication Date: 2006-02-14
    Description: A wide site of potential astronomical and solar system scientific studies using the wide field planetary camera on space telescope are described. The expected performance of the camera as it approaches final assembly and testing is also detailed.
    Keywords: ASTRONOMY
    Type: Space Telescope Science Inst. The Space Telescope Obs.; p 28-39
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  • 3
    Publication Date: 2011-08-12
    Description: Far UV filter observations of main sequence and giant stars analyzed for attainable magnitude accuracy, comparing observations with model atmospheres
    Keywords: SPACE SCIENCES
    Type: ; ECTRON (
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  • 4
    Publication Date: 2011-08-12
    Description: Tungsten filament lamps calibrated against freezing Pt black body for use as standards for stellar spectrophotometry and astronomical radiation measurements
    Keywords: SPACE SCIENCES
    Type: ; ECTRON (
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  • 5
    Publication Date: 2016-06-07
    Description: General results are presented based on nearly completed reductions of data for approximately 35 galaxies of all Hubble types. In general the visual and ultraviolet energy distributions are well correlated. The energy distribution in late-type galaxies appears to turn up sharply in the region around 2000 A, and this is tentatively interpreted as due to the presence of early-type stars whose energy distribution is modified by interstellar dust within these objects. Similar turnups may be present in several elliptical galaxies but the evidence at this time is not definitive.
    Keywords: SPACE SCIENCES
    Type: NASA, Washington The Sci. Results from the Orbiting Astron. Obs. (OAO-2); p 559-574
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  • 6
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    In:  Other Sources
    Publication Date: 2016-06-07
    Description: Filter photometry measurements of the integrated light from several globular clusters between 1500 and 4000 A are discussed. The techniques and problems associated with carrying out photometry of faint extended sources with the OAO-2 instrumentation are described first. The energy distribution for globular clusters determined from these data are corrected for interstellar extinction on the basis of B-V color excesses and a mean ultraviolet extinction curve. The results are compared with synthetic cluster calculations. The ultraviolet energy distribution is primarily determined by the number of stars at the blue end of the horizontal branch.
    Keywords: SPACE SCIENCES
    Type: NASA, Washington The Sci. Results from the Orbiting Astron. Obs. (OAO-2); p 541-558
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  • 7
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    In:  CASI
    Publication Date: 2016-06-07
    Description: The appearance of the bright nova, Nova Serpentis 1970, provided the first opportunity to obtain spectrophotometric observations of a nova in the vacuum ultraviolet. OAO-2 carried out systematic measurements from shortly after outburst on through the first sixty days of nova activity. This data consist of filter photometry and spectral scans. General characteristics of the light and spectral variations in the ultraviolet exhibited by this set of data are described.
    Keywords: SPACE SCIENCES
    Type: NASA, Washington The Sci. Results from the Orbiting Astron. Obs. (OAO-2); p 535-540
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  • 8
    Publication Date: 2016-06-07
    Description: The essential features of the calibration procedure can be divided into three parts. First, the shape of the bandpass of each photometer was determined by measuring the transmissions of the individual optical components and also by measuring the response of the photometer as a whole. Secondly, each photometer was placed in the essentially-collimated synchrotron radiation bundle maintained at a constant intensity level, and the output signal was determined from about 100 points on the objective. Finally, two or three points on the objective were illuminated by synchrotron radiation at several different intensity levels covering the dynamic range of the photometers. The output signals were placed on an absolute basis by the electron counting technique described earlier.
    Keywords: SPACE SCIENCES
    Type: NASA, Washington The Sci. Results from the Orbiting Astron. Obs. (OAO-2) e; p 361-365
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  • 9
    Publication Date: 2016-06-07
    Description: The first observations of a comet in the vacuum ultraviolet were obtained on January 14, 1970, when OAO-2 recorded the spectrum of the bright comet Tago-Sato-Kosaka (1969g). The observations revealed, among other things, the predicted extensive hydrogen Lyman alpha halo. OAO-2 continued to collect spectrophotometric measurements of this comet throughout January of that year; a photograph of the nucleus in Lyman alpha revealed finer scale structures. In February of 1970, the bright comet Bennet (1969i) became favorable for space observations. On the basis of the OAO discovery, OGO-V made several measurements of comet Bennet with low spatial resolution photometers. Comet Enke was detected by OGO in January of 1971 at a large heliocentric distance from its Lyman alpha emission.
    Keywords: SPACE SCIENCES
    Type: NASA, Washington The Sci. Results from the Orbiting Astron. Obs. (OAO-2); p 109-114
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  • 10
    Publication Date: 2019-05-29
    Description: Stellar spectrophotometry in vacuum ultraviolet - feasibility of ultraviolet spectrophotometric satellite, interference filter fabrication, vacuum calibration, and X-15 rocket aircraft
    Keywords: SPACE SCIENCES
    Type: NASA-CR-69482
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