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  • 1
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] The optical counterpart to GRB970228 was observed with the HST Wide Field and Planetary Camera (WFPC2) on 26 March14 and 7 April151997, about 26 and 39 days after the outburst, respectively. The optical counterpart was placed at the centre of the Planetary Camera field of view, so as to attain ...
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 271 (1978), S. 633-634 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Photoelectric photometry of nine stars in a 1 arc min field about Aql X-l was obtained in July and August 1976, using the 2.1 m reflector of the Kitt Peak National Observatory with the Cassegrain computer-photometer. Standardisation of these t/fiFdata was achieved through observations of standard ...
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    Springer
    Space science reviews 74 (1995), S. 101-112 
    ISSN: 1572-9672
    Keywords: Infrared telescopes ; Balloons
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The tropopause, typically at 16 to 18 km altitude at the lower latitudes, dips to 8 km in the polar regions. This makes the cold, dry and nonturbulent lower stratosphere accessible to tethered aerostats. Tethered aerostats can fly as high as 12 km and are extremely reliable, lasting for many years. In contrast to free-flying balloons, they can stay on station for weeks at a time, and payloads can be safely recovered for maintenance and adjustment and relaunched in a matter of hours. We propose to use such a platform, located first in the Arctic (near Fairbanks, Alaska) and, potentially, later in the Antarctic, to operate a new technology 6-meter, diluted aperture telescope with diffraction-limited performance in the near infrared. Thanks to the low ambient temperature (220 K), thermal emission from the optics is of the same order as that of the zodiacal light in the 2 to 3 micron band. Since this wavelength interval is the darkest part of the zodiacal light spectrum from optical wavelengths to 100 microns, the combination of high resolution images and a very dark sky make it the spectral region of choice for observing the redshifted light from galaxies and clusters of galaxies at moderate to high redshifts.
    Type of Medium: Electronic Resource
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