Results 301 to 310 of about 2,093,256 (347)
Some of the next articles are maybe not open access.
The X-Ray Imaging Telescopes on EXOSAT
Space Science Reviews, 1981The instrument configuration and performance characteristics of the X-ray imaging telescopes on EXOSAT are described. The instrument comprises two fully independent Wolter I imaging telescopes. Each telescope can be used in either of two principal modes: (i) an imaging mode with either a position sensitive proportional counter or a channel multiplier ...
P. A. J. de Korte +8 more
openaire +1 more source
Operation of the x-ray telescope eROSITA
SPIE Proceedings, 2010The X-ray telescope eROSITA is the core instrument besides the Russian ART-XC on the Russian Spektrum-Roentgen- Gamma satellite which will be launched in 2012 to an orbit around the L2 point of the Earth-Sun-system. During both survey and pointing phase the solar panels and the antenna constrain the possible mission scenario.
Fürmetz, M. +3 more
openaire +2 more sources
Wolter-Schwarzschild Telescopes for X-Ray Astronomy
Applied Optics, 1973The resolution of a Wolter-Schwarzschild telescope is intrinsically superior to the resolution of the corresponding paraboloid-hyperboloid telescope. The improvement is important for high resolution and wide field telescope designs having grazing angles larger than about 1.5 degrees .
R C, Chase, L P, Vanspeybroeck
openaire +2 more sources
Observation of a Solar Flare at the Limb with the Yohkoh Soft X-Ray Telescope
Nippon Tenmon Gakkai obun kenkyu hokoku, 1992A long-enduring soft X-ray flare at the solar limb was well observed by the Soft X-ray Telescope aboard the Yohkoh spacecraft from its pre-flare stage through the post-flare phase.
S. Tsuneta +6 more
semanticscholar +1 more source
AIP Conference Proceedings, 2003
The Swift Gamma‐Ray Burst Explorer is designed to make prompt multiwavelength observations of Gamma‐Ray Bursts (GRBs) and their afterglows. The X‐ray Telescope (XRT) provides key capabilities that permit Swift to determine GRB positions with several arcsecond accuracy within 100 seconds of the burst onset.
openaire +1 more source
The Swift Gamma‐Ray Burst Explorer is designed to make prompt multiwavelength observations of Gamma‐Ray Bursts (GRBs) and their afterglows. The X‐ray Telescope (XRT) provides key capabilities that permit Swift to determine GRB positions with several arcsecond accuracy within 100 seconds of the burst onset.
openaire +1 more source
Novel X-ray telescopes for wide-field X-ray monitoring
Il Nuovo Cimento C, 2005We report on fully innovative very wide-field of view X-ray telescopes with high sensitivity as well as large field of view. The prototypes are very promising, allowing the proposals for space projects with very wide-field Lobstereye X-ray optics to be considered.
Hudec, R. +3 more
openaire +1 more source
Grazing Incidence X-Ray Telescopes
1969This paper reviews some of the work related to X-ray imaging which has been done at our laboratory over the past several years. Our interest has been to develop high resolution telescopes for studying X-ray emission from the sun and from other celestial X-ray sources.
W. P. Reidy +4 more
openaire +1 more source
The Soft X-ray Telescope for the SOLAR-A mission
, 1991S. Tsuneta +12 more
semanticscholar +1 more source
The X-Ray Telescope (XRT) for the Hinode Mission
, 2007L. Golub +28 more
semanticscholar +1 more source

