Source structure via the occultation technique

Details Source structure via the occultation technique Source structure via the occultation technique

May 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975xrat.rept..159f&link_type=abstract

In ESA X-Ray Astronomy and Related Topics p 159-165 (SEE N76-11958 02-89)

Astronomy and Astrophysics

Astronomy

Esa Satellites, Lunar Occultation, X Ray Sources, Collimators, Radiation Counters, Spaceborne Telescopes, Supernovae, Uhuru Satellite

Scientific paper

Ultimate limitations on measurements of X-ray source structure are considered for the EXOSAT mission. A fundamental lower limit to flux measurements is derived from X-ray source counts available from the Uhuru satellite. Most sources observed have a sufficiently high surface brightness so that confusion will not prove a problem. Limits on the measuring methods of telescopes, modulation collimators, and occultation are mentioned.

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