Max-Planck-Institut für extraterrestrische Physik
Timing
Deutsche Version MPE HEG X-Ray Astronomy Wave ROSAT
Next: Positional Accuracy Up: 6.2 Performance of the Previous: Point Spread Function
Timing
The individual events detected by the WFC are time-tagged to a
resolution of approximately 
by the CDHS,
which allows the scanning motion of the sky survey to be removed
without image degradation due to smearing effects.
There are no EUV sources which are bright enough for this timing
restriction to be a limitation.
If you have problems/suggestions please send mail to xray-info @ mpe . mpg . de