Campaign 8 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, X         A1   +54
  HD 173511   B, Y         K4   +61
  alp Lyr     C (primary)  A1'  +38
  del Scl     D            A1   -28
  HD 166780   E, Z         K4   +57
  HD 15508    F            K0   -68

For a campaign lasting 6 days (plus any fraction), sources should
be observed in the following order:

6-day campaign
  day  sequence

   1   A  B  C 
   2   D  F  Z
   3   X  B  C
   4   D  F  E
   5   A  Y  C
   6   D  F  E
  (7)  A  B 

For campaigns of 4 or 5 days, the following sequences apply:

3.8-day campaign   4-day campaign     5-day campaign
  day  sequence      day  sequence      day  sequence
   1   A  B  Z        1   A  B  C        1   A  B  C
   2   X  F  E        2   X  F  Z        2   D  F  Z
   3   B  F  E        3   B  F  E        3   X  B  E
   4   A  Y           4   A  Y  E        4   D  F  E
                     (5)  A  B           5   A  F  Y
                                        (6)  A  B

Note 1:  In the above schedules, one observation of targets A, B, 
and E has been replaced with one observation of targets X, Y, and
Z, respectively.  These AORs are identical to their replacement
except that they utilize different ramp times.

  target     letters  SL      LL        SH        LH

  HR 5467    A, X     6-14 s  30-120 s  30-120 s
  HD 173511  B, Y             14-30 s   6-30 s    60-240 s
  HD 166780  E, Z                                 14-60 s

Note 2:  The above schedules are tailored specifically to Campaign 8
(to end each day in the north).

Note 3:  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.  The shorter campaigns have already 
eliminated most observations of Star C.

Note 4:  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 5:  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-8A-HR5467    2x14  2x14  2x120   4x120   4x120          8    22   2370
calsfx-8B-HD173511  2x 6  2x 6  2x 30   6x 30   4x 30   8x 60  8    32   1988
calsfx-8C-alpLyr                                6x  6   6x 14  -    12    988
calsfx-8D-delScl    2x 6  2x 6  2x120   4x120   2x120          8    20   2033
calsfx-8E-HD166780  2x 6  2x 6  2x 30   8x 30   4x 30   8x 60  8    34   2066
calsfx-8F-HD15508   2x 6  2x 6  2x 30   8x 30   4x 30   8x 60  8    34   2066
calsfx-8X-HR5467    4x 6  4x 6  8x 30  16x 30  16x 30          8    56   2495
calsfx-8Y-HD173511  2x 6  2x 6  4x 14  12x 14  16x  6   2x240  8    46   2092
calsfx-8Z-HD166780  2x 6  2x 6  2x 30   8x 30   4x 30  32x 14  8    58   2180

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.