Campaign 6 in normal ops will use the following standards. This plan is based on a 6-day campaign. If this is changed, please contact G. Sloan for further instructions. target letter sp. declination HR 5467 A A1 +54 HD 173511 B K4 +61 alp Lyr C (primary) A1' +38 lam Tel D A1 -52 HD 166780 E K4 +57 HD 166207 F K0 +50 For a campaign lasting 6 days (plus any fraction), sources should be observed in the following order: day observation sequence 1 A B C 2 D E F 3 A B C 4 D E F 5 A B C 6 D E F (7) A B NOTE 1: In the event that 18 observing slots are unavailable in this 6-day campaign, one observation of the primary (Star C, alp Lyr) could be eliminated. NOTE 2: Observations of Star C will need to be followed immediately by a short anneal sequence due to its brightness. In the observing table above, an anneal sequence should naturally follow, as Star C is observed at the end of Days 1, 3, and 5. NOTE 3: In order to improve observatory efficiency, the scheduler should feel free to re-arrange the observing schedules above, as long as sources do not move by more than roughly +/- 12 hours, and as long as the spacing between successive observations of the same source remains roughly the same. Observations have been designed so that successive observations of the same source are spaced by roughly 24 hours or more. Observational details DCEs for .................................. total AORNAME root SL2 SL1 LL2 LL1 SH LH PU DCEs T(s) calsfx-6A-HR5467 2x14 2x14 2x120 4x120 4x120 8 22 2370 calsfx-6B-HD173511 2x 6 2x 6 2x 30 6x 30 4x 30 8x 60 8 32 1988 calsfx-6C-alpLyr 6x 6 6x 14 - 12 988 calsfx-6D-lamTel 2x 6 2x 6 2x120 4x120 2x120 8 20 2033 calsfx-6E-HD166780 2x 6 2x 6 2x 30 8x 30 4x 30 8x 60 8 34 2066 calsfx-6F-HD166207 2x 6 2x 6 2x 30 8x 30 4x 30 8x 60 8 34 2066 The number of DCEs is to the left of the "x", and the ramp time (in sec) is to the right. The number of DCEs is the total for each AOR, including both nod positions.