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Ideally the measurements should be done with the moving telescope to be as cloas as possible in the observation condition. Ideally the measurements should be done with the moving telescope to be as close as possible in the observation condition, i.e. to have also the same synchronization signals as during real on-sky observations.

The absorber should lie on the ABBA rack and it has to be moved into the entrance window by hand.

How to proceed

Ideally the measurements should be done with the moving telescope to be as close as possible in the observation condition, i.e. to have also the same synchronization signals as during real on-sky observations.

The absorber should lie on the ABBA rack and it has to be moved into the entrance window by hand. 

   > Pick-up a source  at the requested  elevation (see XEphem)
   pako> source G34.3 /grep /cat ihet
   >>> G34.3           EQ 2000  18:53:18.56  +01:14:58.2  LSR 0.0  FLUX 19.90 0.0 PROJECT CALIB
   pako> source ABSORBER EQ 2000  18:53:18.56  +01:14:58.2  LSR 0.0  FLUX 19.90 0.0 PROJECT CALIB
   pako> onf 8 80

for acceleration tests:
pako> accTest

AbsorberObs (last edited 2010-12-09 14:08:26 by mrt-lx17)