The SCUCD extension contains information on telescope movements. It is slightly different for JIGGLE (MAP and PHOTOM) and SCAN observations. For a JIGGLE observation it has the following format:
STRUCT.MORE.SCUCD <SCUCD_ST>
JIGL_X(64) <_REAL> -2.6883,-5.3457,-8.033999,-13.3797,
... 5.3457,2.6883,0,2.6883,0,2.6883,0,0
JIGL_Y(64) <_REAL> 1.545,3.09,1.545,1.545,3.09,4.635,6.18,
... -9.27,-7.725,-6.18,-4.635,-3.09,0
DEC1 <_REAL> 0
DEC2 <_REAL> 0
LST_STRT(2,4,3,1) <_DOUBLE> 5.6288711444511,5.630383297715,
... 5.6639924748021,5.6623806283313
RA1 <_REAL> 0
RA2 <_REAL> 0
and for a SCAN observation:
STRUCT.MORE.SCUCD <SCUCD_ST>
JIGL_X <_REAL> 0
JIGL_Y <_REAL> 0
DEC1(1,5,1,1) <_REAL> -17.06608,-17.04154,-17.10884,-17.07168,
-17.11085
DEC2(1,5,1,1) <_REAL> -17.03781,-17.09083,-17.04711,-17.11225,
-17.09126
LST_STRT(1,5,1,1) <_DOUBLE> 5.521871430823,5.5231108938446,
... 5.5266851885263,5.5281428875176
RA1(1,5,1,1) <_REAL> 21.16225,21.16618,21.16226,21.1673,
21.16577
RA2(1,5,1,1) <_REAL> 21.16466,21.16197,21.16755,21.1638,
21.16747
WPLATE <_REAL> 0
The full description of these entries follows:
These are the X and Y coordinates of the jiggle pattern in arcsecond offsets. The coordinate frame is given in the SAM_CRDS FITS keyword. They are only used for JIGGLE observations.
This is the local sidereal time of the start of every switch expressed as decimal radians. It has dimensions of N_SWITCHES, N_EXPOSURES, N_INTEGRATIONS, and N_MEASUREMENTS. The current epoch of observation (Modified Julian Date) is calculated from the UTSTART and UTDATE FITS keywords in SCULIB_GET_MJD.
This is the apparent RA and Dec of the start (RA1, DEC1) and end (RA2, DEC2) of the scans in radians. The dimensions are N_SWITCHES, N_EXPOSURES, N_INTEGRATIONS, and N_MEASUREMENTS. The current epoch of observation (Modified Julian Date) is calculated from the UTSTART and UTDATE FITS keywords in SCULIB_GET_MJD.
For polarimetry observations (POLPHOT or POLPMAP) this array contains the waveplate angle for each measurement (where a measurement is defined as a move of the waveplate). It is used by the SURFLIB_FILL_WPLATE routine.
SURF Programming Interface