Overview of the Solution
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The solution to this problem is to allow the observer to control the
configuration of ISOCAM at the beginning and end of an AOT. This is done by
setting the DRK parameter in PGA to special values which are used as flags.
Briefly, in most cases, the observer will need to add dummy off-source
pointings before and after his target, and will need to use special values
of the DRK parameter in all 3 of the observations (both dummies
and the target).
The DRK field in PGA is normally used to specify procedures for dark
measurements. New values for DRKs have been created, which act as
flags to allow control of the instrument mode at the beginning and end
of an AOT, instead of performing a dark measurement. PLEASE NOTE: It
is the observer's responsibility to insure that ISOCAM does not
saturate during the course of his or her observation and that ISOCAM
is left in parallel mode at the end of the observation.
The three most commonly used DRK flags are:
- DRK = 19 Exit the current AOT without changing ISOCAM's
configuration
- DRK = 20 Begin the current AOT in the configuration ISOCAM
was last left in. Exit the AOT in normal parallel mode.
- DRK = 29 Begin the current AOT in the configuration ISOCAM
was last left in and exit without changing mode.
Note that these DRK flags can only be used with concatenated observations.
Any of the special DRK flags can be set in any of the configurations in the
AOT.
Cautions:
-
If you have a concatenated chain in which both LW and SW are used, you
should not use DRK=20 or 29 in an AOT where the the channel is changed
because the startup sequence must be executed.
-
Since solar system observations cannot be concatenated to off-source
pointings, this mechanism can't be used for SSOs.
Next: A Schematic Example
Up: Saturation of LW
Previous: Details of Parallel
Addendum of the ISOCAM Observer's Manual - V1.0
Mon Aug 5 15:50:39 MET DST 1996