Campaign D1 - D2
================

Summary:
The first major activity with the 24um array.  First light observations
for 24um in D1 - this may be the first time we actually see
celestial objects with MIPS!  The first focus test occurs in D2.
Other basic 24um operations checks, such as determining 24um Voffset
values, a check of the onboard SUR algorithm, preliminary photometry
and superresolution AOT validation, and the first dedicated collection
of 24um darks and flats (in photometry mode) will be obtained.


CAID					TIME	TIME	AOR/IER		COOKBOOK
					ALLOC	USED	PRESENT, 	COMPLETE
							VERSION
--------------------------------------------------------------------------------
(D1)
mips-100  24um first light		25	13.1	yes, A6.2	yes
mips-125  24um Voffset adjustment test	10	4.9	prelim, 6.3	yes
mips-900  24um start-up activities	30	19	prelim, 6.1	yes
mips-950  scattered background monitor	30	23.6	yes, 6.5.2	yes
mips-990  24um shut-down activities	12	8.3	prelim, 6.3	yes

(D2)
mips-110  24um SUR algorithm check	51	33	yes, 6.5.2	yes
mips-121  24um focus confirmation	32	29.3	yes, A6.2	yes
mips-320  24um phot./sr. validation	48	24.4	yes, A6.2	yes
mips-900  24um start-up activities	30	19      prelim, 6.1  	yes
mips-910  24um IOC darks		15	7.1	yes, 6.2.9	yes
mips-917  24um phot. flats		10	11.5	prelim, A6.2	yes
mips-917  24um phot. flats		10	11.5	prelim, A6.2	yes
mips-950  scattered background monitor	30	23.6    yes, 6.5.2	yes
mips-990  24um shut-down activities	12	8.3     prelim, 6.3	yes


questions/issues
----------------
MIPS-110: Failure is critical - the SUR algorithm must be verified,
	  as most 24um science data will be SUR.
	  IER listed in cookbook is different from the linked version
	  (6.1.2 vs. 6.5.2, only 1 second difference in execution time)
	  Why is there a HUGE (13.5 hours!!) slew tax in the newer
	  version of the IER????

MIPS-121: Sensitive to the possible lack of pointing information?
	  (Cluster mode obs.)
	  MIPS-115 listed as a dependency, but this does not occur
	  until one day later in Campaign E!  Results are very
	  dependent on good flats, the very first of which will be
	  obtained concurrently.
	  The same task is in campaign E; however, there is not
	  enough time (1 day) in which to make substantive changes,
	  should a failure occur here.

MIPS-125: Failure is critical, since it affects the entire
	  24um calibration.  Voffsets can be checked in contingency
	  by using other data; however, no appropriate RAW data
	  will be taken until task 110 4 days later (there are no
	  RAW darks, though).

MIPS-320: The AOR included in the cookbook is from Aire version 6.1,
	  while the linked version is from 6.2.
	  MIPS-100 is listed as a dependency - is this really necessary?
	  Is first light actually crucial to anything else?
	  Not entirely clear why an additional 3 cycles of 3s exposures
	  will be taken.  Is this just to confirm that the # of cycles
	  parameter operates correctly?

MIPS-917: Why is this 2 separate tasks?  The positions are the same.
	  Exceeds allotted time.