High resolution large area modular array of reflectors /LAMAR/ Wolter type I X-ray telescope for Spacelab
Abstract
The Spacelab Wolter type I X-ray telescope, which is intended for both astronomical observations and the functional verification of the future Large Area Modular Array of Reflectors (LAMAR) concept, comprises five mirrors and is designed to have a blur circle radius of 20 arcsec, with effective areas of (1) 400 sq cm at 0.25 keV, (2) 200 sq cm in the 0.5-2.0 keV range, and (3) 50 sq cm between 2 and 5 keV. A rotary interchange mechanism allows either of two imaging proportional counters to be placed at the telescope focus. The telescope's primary objective is the observational study of galactic and extragalactic X-ray sources, extending the work of the Einstein Observatory to fainter sources and higher energies. Secondarily, the costs and performance to be expected from the use of this telescope type in the LAMAR mission will be assessed.
- Publication:
-
Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series
- Pub Date:
- 1982
- DOI:
- 10.1117/12.965784
- Bibcode:
- 1982SPIE..284..169C
- Keywords:
-
- Spaceborne Telescopes;
- Spacelab Payloads;
- X Ray Telescopes;
- Flight Operations;
- Galaxies;
- High Resolution;
- Mirrors;
- Performance;
- Structural Design;
- X Ray Sources;
- Astronomy