Campaign 7 in Normal Ops will use the following standards. This plan is based on any campaign length between 4 and 7 days. target letter sp. declination HR 5467 A A1 +54 HD 173511 B K4 +61 bet UMi C (primary) K4' +74 29 Vul D A0 +21 HR 6348 E K0 +60 HD 15508 F K4 -68 HD 55151 G K0 -69 HR 5467 W A1 +54 HR 6348 X K0 +60 HR 5467 Y A1 +54 HD 269352 Z K5 -68 4-day schedule: 5-day schedule day observation sequence day observation sequence 1 A B C 1 A B C 2 D E C 2 D E C 3 A B E 3 A B D 4 W B D 4 D B E (5) C D 5 W E C (6) A B extra: X,Y,Z extra: Y,Z 6-day schedule: 7-day schedule day observation sequence day observation sequence 1 A B C 1 A B C 2 D F E 2 D F E 3 A B C 3 A G B 4 D F E 4 D E C 5 W B C 5 F G D 6 D F E 6 W B C (7) A B 7 G F E (8) A B extra: Y,Z extra: Y,Z Note 1: The third observation of Target A has been replaced with Target W in all schedules. Target W is identical to Target A, except that it uses Red Peak-Up instead of Blue Peak-Up. Note 2: Target Y is a 453-second CHEAP observation, and it can be observed at any time during the campaign. Note 3: Target Z is a 5621-second SPITE AOR. It can be observed any time during the campaign after 0000 13 May 2004 (UT). Before this time, the 1 degree/day rotation of the slit will invalidate the purpose of the observation. Note 4: Target X should only be observed in a four-day campaign. It is identical in every way to Target E, and it can be observed at any time during the campaign. Note 5: In the event that that a single observation must be eliminated, this should be one observation of the primary (Target C, bet UMi). Note 6: Observations of Star C will need to be followed immediately by a short anneal sequence due to its brightness. In all four schedules, this should happen naturally, since it is observed only at the end of a given 24-hour period. Note 7: 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. Note 8: These schedules are specific to Campaign 7 Observational details DCEs for .................................. total AORNAME root SL2 SL1 LL2 LL1 SH LH PU DCEs T(s) calsfx-7A-HR5467 2x14 2x14 2x120 4x120 4x120 8 22 2370 calsfx-7B-HD173511 2x 6 2x 6 2x 30 6x 30 4x 30 8x 60 8 32 1988 calsfx-7C-betUMi 6x 6 6x 6 8 20 988 calsfx-7D-29Vul 2x 6 2x 6 2x120 4x120 4x120 8 22 2333 calsfx-7E-HR6348 2x 6 2x 6 2x 30 8x 30 4x 30 8x 60 8 34 2066 calsfx-7F-HD15508 2x 6 2x 6 2x 30 8x 30 4x 30 8x 60 8 34 2066 calsfx-7G-HD55151 2x 6 2x 6 2x 30 8x 30 4x 30 8x 60 8 34 2066 calsfx-7W-HR5467 2x14 2x14 2x120 4x120 4x120 8 22 2369 calsfx-7X-HR6348 2x 6 2x 6 2x 30 8x 30 4x 30 8x 60 8 34 2066 calsfx-7Y-HR5467 2x 6 - 2 453 calsfx-7Z-HD269352 50x14 8 108 5621 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.