Campaign Q ========== Summary: Contains many detailed or follow-up characterization tasks. Verification of the expected scaling of 24um and 160um darks with exposure time, and a comparison of flat/IC quality versus mirror position, will be done here. Other tasks include the first fine FPS for 24um and 70um WF, validation of the scan AOT (slow speed), throughput measurements for different modes, a very long test to measure off-axis glints, and a large planetary nebula or supernova remnant scan map. CAID TIME TIME AOR/IER COOKBOOK ALLOC USED PRESENT, COMPLETE VERSION -------------------------------------------------------------------------------- mips-905 start-up activities 35 27.1 prelim, 6.3.0 yes mips-930 Ge anneal & recovery 12 6.3 prelim, 6.5.2 prelim mips-912 IOC darks, 160um 15 16.5 yes, 6.2.2 yes mips-911 IOC darks, 70um 30 32.6 yes, 6.2.2 yes mips-910 IOC darks, 24um 15 7.1 yes, 6.2.9 yes mips-190 24um dark verification 21 7.1 yes, 6.2.9 yes mips-192 160um dark verification 16 20.9 yes, 6.2.9 yes mips-307 160um detailed IC, scan 66 65.6 prelim, A6.2 yes mips-306 70um detailed IC, scan 66 65.6 prelim, A6.2 yes mips-305 24um detailed flat, scan 66 65.6 prelim, A6.2 yes mips-930 Ge anneal & recovery 12 6.3 prelim, 6.5.2 prelim mips-924 160um flux standards 20 11.2 yes, A6.2 yes mips-920 24um flux standards 11 7.0 yes, A6.2,6.5 yes mips-922 70um flux standards 12 6.6 yes, A6.2 yes mips-285 scan map of PN or SNR 125 ? no no mips-930 Ge anneal & recovery 12 6.3 prelim, 6.5.2 prelim mips-150 obs. mode rel. throughputs 180 134.2 yes, A6.2 yes mips-930 Ge anneal & recovery 12 6.3 prelim, 6.5.2 prelim mips-328 scan valid., slow speed 450 442.3 yes, A6.2 prelim mips-930 Ge anneal & recovery 12x3 6.3x3 prelim, 6.5.2 prelim mips-317 off-axis glints 900 499.0 yes, A6.2 yes mips-930 Ge anneal & recovery 12x5 6.3x5 prelim, 6.5.2 prelim mips-133 70um WF fine FPS 252 107.4 prelim, 6.5.2 prelim mips-930 Ge anneal & recovery 12 6.3 prelim, 6.5.2 prelim mips-131Q 24um fine FPS 402 166.6 prelim, 6.5.2 prelim mips-235Q 160um fine FPS *newly added* -- 375 no no mips-992 shut-down activities 19 18.5 prelim, 6.3.0 yes total: 2845 2157.8+ questions/issues ---------------- mips-131_Q: Under-budget by almost 4 hours. IER is done twice - why are the times slightly different? No calibration dependencies specified - high-quality flat field must be essential, also need darks. Target included in IER, but not specified in cookbook. mips-133: Under-budget by over 2 hours. No calibration dependencies given - again, must need good flat. Target included in IER, but not specified in cookbook. Has it been vetted for background? mips-150: Includes obs. of 70um WF phot., scan, TP, and SED, but what about fine scale? Cookbook needs a bit more detail. The only task dependency listed is MIPS-322 (70um phot valid.), but it must also need phot. validation for the other 2 arrays, plus scan map, TP, and SED mode AOT validation. mips-305: Any task dependencies? Probably need to have the routine scan flats for comparison. Cookbook asks what the header keyword for the scan mirror position is. Is flat test using standards necessary for this task (i.e., comparing the flat per mirror position to the nominal flat may be all that is required here)? If so, cookbook needs to specify standard star datasets to be used (probably the flux standards taken during this campaign are sufficient). mips-306: Same comments as 305. mips-307: Same comments as 305. mips-317: Under-budget by over 6 hours. Why are the 2 maps at the cross-scan position of the bright source done with medium scan rate, while the rest is fast? This task overlaps somewhat with the ultimate scattered light task (mips-340), which maps a much smaller region (~15') around a bright source . mips-328: Target is a GTO target - conflict? Visibility ends 1 month after the nominally-scheduled time. For the 6-deg. leg scan, will there be enough sources far from cluster to accurately compute positions along entire scan leg? mips-920-924: Are there previous tasks that check any dependencies of the flux conversion factor with exposure time? mips-930: Are the five sets of this listed after MIPS-317 supposed to be interspersed with that task? And similarly for the three sets listed after MIPS-328? The last one, before MIPS-131_Q, doesn't seem necessary, since there is no further Ge data taken. IER only does 160um.