#  Please edit this file with care to maintain the
#  correct format so that SPOT can still read it.
#  Generated by SPOT on:  7/7/2003     13:39:47

HEADER: FILE_VERSION=7.0, STATUS = PROPOSAL

      AOT_TYPE:  MIPS Photometry
     AOR_LABEL:  MIPS-100-0000
    AOR_STATUS:  new

 MOVING_TARGET:  NO
   TARGET_TYPE:  FIXED SINGLE
   TARGET_NAME:  HD 53501
  COORD_SYSTEM:  Equatorial  J2000
      POSITION:  RA_LON=6h59m50.54s,  DEC_LAT=-67d54m59.2s, PM_RA=-0.027", PM_DEC=0.234"
OBJECT_AVOIDANCE:  EARTH = YES, OTHERS = YES

    MICRON_24: FIELD_SIZE = SMALL, EXPOSURE_TIME = 3, N_CYCLES = 2
SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO
RESOURCE_EST: TOTAL_DURATION=349.4, SLEW_TIME=7.2, SETTLE_TIME=5.0, SLEW_OVERHEAD=180.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=594, DOWNLINK_VOLUME=2537774, VERSION=S7.5.1
INTEGRATION_TIME: MIPS_24=92.27469,MIPS_70=0.0,MIPS_160=0.0

COMMENT_START: 
This is the first light observation at 24um.  These data will be used
to confirm system throughput, image quality, and CSMM operation.
COMMENT_END: 







      AOT_TYPE:  MIPS Photometry
     AOR_LABEL:  MIPS-100-0001
    AOR_STATUS:  new

 MOVING_TARGET:  NO
   TARGET_TYPE:  FIXED CLUSTER - OFFSETS
   TARGET_NAME:  HD 53501 - offset
  COORD_SYSTEM:  Equatorial  J2000
     POSITION1:  RA_LON=6h59m50.54s,  DEC_LAT=-67d54m59.2s, PM_RA=-0.027", PM_DEC=0.234"
     OFFSET_P2:  EAST_ROW_PERP=-30.0",	NORTH_COL_PARA=0.0"
OFFSETS_IN_ARRAY:  YES
OBSERVE_OFFSETS_ONLY:  YES
OBJECT_AVOIDANCE:  EARTH = YES, OTHERS = YES

    MICRON_24: FIELD_SIZE = LARGE, EXPOSURE_TIME = 3, SKY_OFFSET = 60.0, N_CYCLES = 2
SPECIAL: IMPACT = none, LATE_EPHEMERIS = NO,SECOND_LOOK = NO
RESOURCE_EST: TOTAL_DURATION=437.022, SLEW_TIME=9.6, SETTLE_TIME=15.222016, SLEW_OVERHEAD=180.0, SPECIAL_OVERHEAD=0.0, UPLINK_VOLUME=799, DOWNLINK_VOLUME=3722068, VERSION=S7.5.1
INTEGRATION_TIME: MIPS_24=67.108864,MIPS_70=0.0,MIPS_160=0.0

COMMENT_START: 
This is the first light observation at 24um.  These data will be used
to confirm system throughput, image quality, and CSMM operation.  The sky
offset is deliberately kept small enough that the star should still be on
the array and can be used to verify the in-scan spacecraft offset.
The target was defined to include an offset half the size of the sky
offset used for the background field, so that the two sets of star
images should be centered in the final mosaic.
COMMENT_END: