Campaign 13 in normal ops will use the following standards. This plan is based on a campaign with a length of 8 to 10 days. target letter sp. F_12 (Jy) dec. del UMi A A1n 0.80 +86 HD 173511 B K4 1.19 +61 alp Lyr C (primary) A0' 41.6 +38 HR 6348 D K0 1.15 +61 HR 7018 E A0 0.20 +63 HD 39577 F K2 0.56 -55 HD 23593 G K3 1.07 -64 HD 19241 H K5 1.25 -60 HD 50160 I K2 0.52 -57 ksi Dra J (primary) K2' 16.85 +56 HR 7018 V A0 0.20 +63 HD 19241 W K5 1.25 -60 For a campaign lasting 8-10 days (plus any fraction), sources should be observed in the following order: 8-day campaign 9-day campaign 10-day campaign day sequence day sequence day sequence 1 A B 1 A B 1 A B 2 D C 2 D C 2 D C 3 F E 3 F E 3 F E 4 G A 4 G A 4 G A 5 H B 5 H B 5 H B 6 F D 6 F 6 I 7 W V 7 V D 7 F V 8 G B 8 W A 8 G D (9) A 9 G B 9 W A (10) J 10 I B (11) J Note 1: In the above schedules, one observation of targets E and H has been replaced with one observation of targets V and W, respectively. These AORs are identical to those which they are replacing, except that target V uses Blue PU and target W uses PCRS PU instead of the usual Red PU. Note 2: The above schedules are tailored specifically to Campaign 13 (to end each day in the north). Note 3: The one observation of target C will need to be followed immediately by a short anneal sequence due to its brightness. This should happen naturally, as target C is the last target on Day 2. Note 4: 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-13A-delUMi 2x 6 2x 6 2x 30 8x 30 6x 30 8 28 1506 calsfx-13B-HD173511 2x 6 2x 6 2x 30 6x 30 4x 30 8x 60 8 32 1988 calsfx-13C-alpLyr 6x 6 6x 14 - 12 992 calsfx-13D-HR6348 2x 6 2x 6 2x 30 8x 30 4x 30 8x 60 8 34 2066 calsfx-13E-HR7018 2x14 2x14 2x120 4x120 4x120 8 22 2369 calsfx-13F-HD39577 2x 6 2x 6 4x 30 12x 30 6x 30 8 34 1738 calsfx-13G-HD23593 2x 6 2x 6 2x 30 8x 30 4x 30 8x 60 8 34 2066 calsfx-13H-HD19241 2x 6 2x 6 2x 30 6x 30 4x 30 8x 60 8 32 1988 calsfx-13I-HD50160 2x 6 2x 6 4x 30 12x 30 6x 30 8 34 1739 calsfx-13J-ksiDra 6x 6 6x 60 - 12 1243 calsfx-13V-HR7018 2x14 2x14 2x120 4x120 4x120 8 22 2370 calsfx-13W-HD19241 2x 6 2x 6 2x 30 6x 30 4x 30 8x 60 - 28 1968 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: 13 Aug 04)