Campaign 3 in normal ops will use the following standards.  This plan
is based on a 5.5-day campaign.  If it is shortened to 4 days, sources
H and I should be dropped.  Source J has been added in the (unlikely)
event that the campaign covers 6 full days for calibration purposes.


  target      letter      declination

  del UMi     A           +86
  HD 173511   B           +61
  eps Car     C (primary) -59
  HR 4138     D           -71
  HR 6606     E           +61
  tau Cen     F           -48
  HD 108599   G           -16
  ksi1 Cen    H           -49
  HD 30895    I           -56
  HD 130499   J           +56

If the campaign lasts 4 days (plus any fraction), sources should
be observed in the following order:

  day  observation sequence

   1   A  B  C  A  D  E    
   2   A  B  F  G  D  C    
   3   A  B  E  F  G  C    
   4   A  B  E  F  G  D    
  (5)  A  B  C  D  E   

If the campaign lasts 5 days (plus any fraction), sources should
be observed in the following order:

  day  observation sequence

   1   A  B  C  D  F  E    
   2   A  G  B  H  I  C    
   3   A  D  B  F  G  E    
   4   A  H  C  I  D  B    
   5   G  F  A  I  H  E    
  (6)  A  B  C  D  E       


If the campaign lasts 6 days (plus any fraction), sources should
be observed in the following order:

  day  observation sequence

   1   A  B  C  D  F  E    
   2   A  G  B  H  I  J    
   3   A  B  C  D  F  E    
   4   A  G  B  H  I  J    
   5   A  B  C  D  F  E    
   6   A  G  B  H  I  J    
  (7)  A  B  C  D  E

The 5-day and 6-day tables apply specifically to Campaign 3 and should 
not be used for other campaigns.

NOTE:  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.
The exception to this rule is when a source is scheduled for two
observations in a 24-hour period (e.g. source A, 4-day campaign, day 1).

Observational details

                    DCEs for ..................................  total
AORNAME root        SL2   SL1   LL2    LL1    SH     LH      PU  DCEs  T(s)

calsfx-3A-delUMi    2x 6  2x 6  2x 30  8x 30  6x 30          8    28   1514
calsfx-3B-HD173511  2x 6  2x 6  2x 30  6x 30  4x 30   8x 60  8    32   2005
calsfx-3C-epsCar                                      6x 14  -     6    787
calsfx-3D-HR4138    2x 6  2x 6  2x120  4x120  2x120          8    20   2036
calsfx-3E-HR6606    2x 6  2x 6  2x 14  6x 14  2x 30   8x 60  8    30   1807
calsfx-3F-tauCen    2x 6  2x 6  2x 14  8x 14  4x 30   8x 60  8    34   1911
calsfx-3G-HD108599  2x 6  2x 6  2x 30  8x 30  6x 30   8x 60  8    36   2155
calsfx-3H-ksi1Cen   2x 6  2x 6  2x120  4x120  2x120          8    20   2036
calsfx-3I-HD30895   2x 6  2x 6  2x 30  6x 30  4x 30   8x 60  8    32   2009
calsfx-3J-HD130499  2x 6  2x 6  2x 30  6x 30  6x 30   8x 60  8    34   2156

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.