Modifications were made to the X-ray reflectometer located at the Space Sciences Laboratory, Marshall Space Flight Center. One was an automatic drive for the Large Micrometer Head. This system, interfaced with the Hewlett Packard Computer System, is used to record data and provides the X-ray reflectometer with an automated data-taking capability. Using this system, a complete scatter curve can be obtained automatically. Previously, it was necessary to manually reset the system after recording for each data point in the scatter curve. The second modification provided an externally controlled electrical drive to move the microfocus X-ray source along its axis. With this modification, one can translate the X-ray source while it is operating to...
In order to test the instruments aboard the Advanced X-ray Astrophysics Facility (AXAF) some modific...
Data obtained during five nights of continuous monitoring of the X-ray source Seo X-1 between April ...
Data obtained during five nights of continuous monitoring of the X-ray source Seo X-1 between April ...
The results from an experimental program to determine the reflection efficiency and scatter paramete...
Optical surfaces built for X-ray telescopes are made to reflect very short wavelengths that range in...
In investigating the dispersion properties of telescope mirrors used in X-ray astronomy, the slight ...
X-ray astronomy was born on 1962 when Giacconi decided to put a Geiger counter onto a rocket, in hop...
X-ray astronomy was born on 1962 when Giacconi decided to put a Geiger counter onto a rocket, in hop...
Data on the scattering of X-rays from various mirror flats obtained from different vendors. The scat...
Particulate contamination on astronomical mirrors degrades performance in two ways: by information l...
The results of a ray-trace analysis of several glancing-incidence X-ray optical systems are presente...
The testing is reported of a polished Kanigen coated beryllium mirror in a soft X-ray telescope to b...
NASA's Chandra X-ray Observatory includes a Flight Contamination Monitor (FCM), a system of 16 radio...
The use of microchannel plates as focal plane readout devices and the evaluation of mirrors for X-ra...
X-ray collectors and detectors evaluated for use as spectrography experiment in Orbiting Astronomica...
In order to test the instruments aboard the Advanced X-ray Astrophysics Facility (AXAF) some modific...
Data obtained during five nights of continuous monitoring of the X-ray source Seo X-1 between April ...
Data obtained during five nights of continuous monitoring of the X-ray source Seo X-1 between April ...
The results from an experimental program to determine the reflection efficiency and scatter paramete...
Optical surfaces built for X-ray telescopes are made to reflect very short wavelengths that range in...
In investigating the dispersion properties of telescope mirrors used in X-ray astronomy, the slight ...
X-ray astronomy was born on 1962 when Giacconi decided to put a Geiger counter onto a rocket, in hop...
X-ray astronomy was born on 1962 when Giacconi decided to put a Geiger counter onto a rocket, in hop...
Data on the scattering of X-rays from various mirror flats obtained from different vendors. The scat...
Particulate contamination on astronomical mirrors degrades performance in two ways: by information l...
The results of a ray-trace analysis of several glancing-incidence X-ray optical systems are presente...
The testing is reported of a polished Kanigen coated beryllium mirror in a soft X-ray telescope to b...
NASA's Chandra X-ray Observatory includes a Flight Contamination Monitor (FCM), a system of 16 radio...
The use of microchannel plates as focal plane readout devices and the evaluation of mirrors for X-ra...
X-ray collectors and detectors evaluated for use as spectrography experiment in Orbiting Astronomica...
In order to test the instruments aboard the Advanced X-ray Astrophysics Facility (AXAF) some modific...
Data obtained during five nights of continuous monitoring of the X-ray source Seo X-1 between April ...
Data obtained during five nights of continuous monitoring of the X-ray source Seo X-1 between April ...