Campaign 9 in normal ops will use the following standards. This plan is based on a campaign with a length of 4 to 6 days. target letter sp. declination HR 5467 A A1 +54 HD 173511 B K4 +61 alp Lyr C (primary) A1' +38 alp Lac D A1 +50 HR 6348 E K0 +61 HD 99754 F K4 -23 HD 55151 G K0 -65 For a campaign lasting 4-6 days (plus any fraction), sources should be observed in the following order: 4-day campaign 5-day campaign 6-day campaign day sequence day sequence day sequence 1 A B C 1 A B C 1 A B C 2 D A E 2 D F E 2 D F E 3 B A D 3 A B D 3 A G B 4 E B D 4 E F D 4 D F E (5) A B 5 A B E 5 A G B (6) A B 6 D F E (7) A B Note 1: The above schedules are tailored specifically to Campaign 9 (to end each day in the north). Note 2: The one observation of Star C will need to be followed immediately by a short anneal sequence due to its brightness. This should happen naturally, as Star C is the last target on Day 1. 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-9A-HR5467 2x14 2x14 2x120 4x120 4x120 8 22 2370 calsfx-9B-HD173511 2x 6 2x 6 2x 30 6x 30 4x 30 8x 60 8 32 1988 calsfx-9C-alpLyr 6x 6 6x 14 - 12 988 calsfx-9D-alpLac 2x 6 2x 6 2x 30 4x 30 4x 30 8 22 1271 calsfx-9E-HR6348 2x 6 2x 6 2x 30 8x 30 4x 30 8x 60 8 34 2066 calsfx-9F-HD99754 2x 6 2x 6 2x 30 8x 30 4x 30 8x 60 8 34 2066 calsfx-9G-HD55151 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. (Version date: 17 May 04)