The Ultraviolet Imaging Telescope (UIT) was designed and built at NASA's Goddard Space Flight Center in Greenbelt, Maryland. Collection Item Summary: This is part of a suite of flight cabling for the ultraviolet 36-inch reflecting telescope known as HUT (Hopkins Ultraviolet Telescope), one of the three main instruments designed to observe the sky in the ultraviolet and x-ray regions of the spectrum on … The concept, for a 0.9 m telescope to fly multiple times on the space shuttle as an attached payload, was a direct descendant of the rocket program at JHU. The Hopkins Ultraviolet Telescope (HUT) was a NASA-funded telescope whose specialized purpose was to explore the Universe using the technique of low-resolution spectroscopy in the far-ultraviolet (850 - 1850 Angstrom) spectral region. The Hopkins Ultraviolet Telescope (HUT) was a space telescope designed to make spectroscopic observations in the far-ultraviolet region of the electromagnetic spectrum.It was flown into orbit on the Space Shuttle and operated from the Shuttle's payload bay on two occasions: in December 1990, as part of Shuttle mission STS-35, and in March 1995, as part of mission STS-67. The Hopkins Ultraviolet Telescope (HUT; Davidsen et al. The Astro UV payload consisted of UIT, the Hopkins Ultraviolet Telescope (HUT), and the Wisconsin Ultraviolet Photo-Polarimeter Experiment (WUPPE).
WUPPE was a UV spectro-polarimeter (University of Wisconsin, led by A. D. Code). The Hopkins Ultraviolet Telescope (HUT), part of the Astro 2 Observatory that flew aboard the space shuttle last March (SN: 3/4/95, p.133), recorded a series of such gaps in the spectrum of the quasar HS1700+64, which lies about 10 billion light-years from Earth. This is the first spectrum of Her X-1 that extends down to the Lyman limit at 912 ˚A. The Hopkins Ultraviolet Telescope (HUT) project was accepted for development by NASA. Hubble’s images are limited only by the telescope’s engineering and the properties of light itself. The project grew out of the JHU sounding rocket program. We have obtained a far-ultraviolet spectrum of the X-ray binary Hercules X-1/HZ Herculis using the Hopkins Ultraviolet Telescope aboard the Astro-1 space shuttle mission in 1990 December.
This 0.4 meter telescope with a UV-sensitive image intensifier carried 2-1000 frame cassettes of 70mm IIa-O astronomical film and was used to image 40 arcminute circular fields of view with about 2 arcsecond resolution. Hubble's images reveal the complex, three-dimensional structure of galaxies, nebulae and star-forming regions with incredible acuity, chiefly because the telescope is in space.
1992) was a 0.9 m telescope and moderate-resolution (Δλ ¼ 3 Å) far-ultraviolet (FUV) prime-focus Rowland-circle spectro-graph developed and built by the Johns Hopkins University (JHU) under the leadership of Professor Arthur F. Davidsen.
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WUPPE was a UV spectro-polarimeter (University of Wisconsin, led by A. D. Code). The Hopkins Ultraviolet Telescope (HUT), part of the Astro 2 Observatory that flew aboard the space shuttle last March (SN: 3/4/95, p.133), recorded a series of such gaps in the spectrum of the quasar HS1700+64, which lies about 10 billion light-years from Earth. This is the first spectrum of Her X-1 that extends down to the Lyman limit at 912 ˚A. The Hopkins Ultraviolet Telescope (HUT) project was accepted for development by NASA. Hubble’s images are limited only by the telescope’s engineering and the properties of light itself. The project grew out of the JHU sounding rocket program. We have obtained a far-ultraviolet spectrum of the X-ray binary Hercules X-1/HZ Herculis using the Hopkins Ultraviolet Telescope aboard the Astro-1 space shuttle mission in 1990 December.
This 0.4 meter telescope with a UV-sensitive image intensifier carried 2-1000 frame cassettes of 70mm IIa-O astronomical film and was used to image 40 arcminute circular fields of view with about 2 arcsecond resolution. Hubble's images reveal the complex, three-dimensional structure of galaxies, nebulae and star-forming regions with incredible acuity, chiefly because the telescope is in space.
1992) was a 0.9 m telescope and moderate-resolution (Δλ ¼ 3 Å) far-ultraviolet (FUV) prime-focus Rowland-circle spectro-graph developed and built by the Johns Hopkins University (JHU) under the leadership of Professor Arthur F. Davidsen.
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