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The Far Ultraviolet Background: Dust Scattering and the Extragalactic Continuum

Published online by Cambridge University Press:  08 February 2017

Mark Hurwitz ,
Stuart Bowyer  and
Christopher Martin
Mark Hurwitz
Affiliation:
Center for EUV Astrophysics University of California Berkeley, CA 94720 USA
Stuart Bowyer
Affiliation:
Center for EUV Astrophysics University of California Berkeley, CA 94720 USA
Christopher Martin
Affiliation:
Physics Department Columbia University New York, NY 10027 USA

Extract

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NASA's Ultraviolet Experiment (UVX) payload, which flew aboard space shuttle Columbia in January 1986, contained a spectrograph built by the Space Astrophysics Group at the University of California, Berkeley. The wavelength range is 1400–1850 Å with a FWHM resolution of ~15 ± 2 Å. A full description of the instrument can be found in Martin and Bowyer (1984). The instrument was pointed at various regions of the sky for 8 nighttime orbits. Targets spanning a wide range of galactic latitudes and neutral hydrogen column densities were observed.

Type
III. Diffuse Galactic Radiation from Dust and Gas: Observations and Models
Information
Symposium - International Astronomical Union , Volume 139: The Galactic and Extragalactic Background Radiation , 1990 , pp. 229 - 230
Copyright
Copyright © Kluwer 1990 

References

REFERENCES

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