The Deep Survey Dead Spot is a region of lowered sensitivity
(ie localized gain decrease) caused by a very high
flux density of the bright EUV source, HZ 43.
The January, 1993 observation on boresight focused light onto
a very few microchannels.
The resulting deadspot is a region roughly 800 microns (1.7 arcmin FWHM)
in diameter with a very low response.
Deep Survey count rates are attenuated by up to 75% by the DS Dead Spot.
A sensitivity map of the DS detector is constructed from Moon observations
and is used for count rate corrections.
Under certain conditions, countrates are restored to
+/- 15% of their expected value.
The Memo included below describes the dead spot and a corrective algorithm.
Note from DC: I don't think people have had much luck in correcting
Deep Survey images/light curves. The pixel-to-pixel variations
are too great. The EUVE reference package includes a pixel Mask
for the Dead Survey Lexan region (ds_dead.pl), but using this mask
also throws away many good photons.
In 1997 EUVE lowered the lower-level discrimantor
for the DS, which means that events from the region of low gain
could be recovered using pulse-height filtering. However, this is
only true in WSZ telemetry mode (which was used infrequently back in 93/94).