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SIMPLE  =                    T / Fits standard
BITPIX  =                  -32 / Bits per pixel
NAXIS   =                    2 / Number of axes
NAXIS1  =                 2040 / Axis length
NAXIS2  =                 2044 / Axis length
ORIGIN  = 'KPNO-IRAF'          / FITS file originator
DATE    = '2003-02-12T18:01:52' / Date FITS file was generated
IRAF-TLM= '15:01:08 (29/08/2001)' / Time of last modification
DATAMIN =          -4.532102E7 / Minimum data value
DATAMAX =           1.307323E7 / Maximum data value
EXTEND  = 'F         '         /FILE MAY HAVE EXTENSIONS
OBJECT  = 'NGC 4038 I'         /TARGET NAME
IRAFNAME= 'ccd5084 '           /NAME OF IRAF IMAGE FILE
IMAGE   = 'NGC4038/39'         /IMAGE NAME
IRAF-MAX=             32767.00 /DATA MAX
IRAF-MIN=                 0.00 /DATA MIN
IRAF-BPX=                   32 /DATA BITS/PIXEL
IRAFTYPE= 'REAL    '           /PIXEL TYPE
OBSERVAT= 'Las Campanas'       /OBSERVATORY
OBSERVER= 'Madore & Parker'    /OBSERVERS
EXPTIME =               600.00 /ACTUAL INTEGRATION TIME
DARKTIME=              -999.00 /TOTAL ELAPSED TIME
IMAGETYP= '_         '         /OBJECT, DARK, BIAS, ETC.
DATE-OBS= '21/12/95'           /DATE (DD/MM/YY) OF OBS.
UT      = '06 57 48'           /UNIVERSAL TIME
ZD      = '_         '         /ZENITH DISTANCE
AIRMASS =              1.65000 /AIRMASS RANGE: 1.65-1.50?
FILTER  = 'I       '           /FILTER NAME
TELESCOP= 'Dupont 100 in'      /TELESCOPE NAME
DETECTOR= 'TEK5    '           /DETECTOR
GAIN    =                 2.00 /GAIN, ELECTRONS PER ADU
RDNOISE =                 5.80 /READ NOISE, ELECTRONS
CCDSEC  = '[3:2042,3:2046]'    /ORIENTATION TO FULL FRAME
ORIGSEC = '_         '         /ORIGINAL SIZE FULL FRAME
CCDSUM  = '1 1       '         /ON CHIP SUMMATION
INSTRUME= '_         '         /INSTRUMENT
TRIM    = 'Jan 24 16:49 Trim data section is [3:2042,3:2046]' /
OVERSCAN= 'Jan 24 16:49 Overscan section is [2050:2060,1:2048] with mean=596.98'
ZEROCOR = 'Jan 24 16:49 Zero level correction image is Zero5' /
FLATCOR = 'Jan 24 16:49 Flat field image is FlatI5 with scale=18113.36' /
ILLUMCOR= '_         '         /
CCDPROC = 'Jan 24 16:50 CCD processing done' /
NCOMBINE=                    1 /
EQUINOX =              2000.00 /EQUINOX OF REF. COORD.
CTYPE1  = 'RA---TAN'           /COORDINATE TYPE
CTYPE2  = 'DEC--TAN'           /COORDINATE TYPE
BUNIT   = 'ADU       '         /FLUX UNIT SCALE
CRPIX1  =              1020.50 /REFERENCE PIXEL IN LINES
CRPIX2  =              1022.50 /REFERENCE PIXEL IN SAMPLES
CRVAL1  =             180.4733 /R.A. (DEGREES)
CRVAL2  =             -18.8780 /DEC  (DEGREES)
CD1_1   =         -7.22075E-05 /DEGREES/PIXEL
CD2_1   =          1.54805E-06 /DEGREES/PIXEL
CD1_2   =          1.74413E-06 /DEGREES/PIXEL
CD2_2   =          7.21714E-05 /DEGREES/PIXEL
RA      = '  12 01 53.6'       /RIGHT ASCENSION (HRS MIN SEC)
DEC     = ' -18 52 40.7'       /DECLINATION     (DEG MIN SEC)
PIXELSIZ=                0.260 /PIXEL SIZE (ARCSECONDS)
DSCALE  =          1.00000E+00 /
DZERO   =          0.00000E+00 /
SEEING  =              -999.00 /SEEING (ARCSECONDS)
PHOTOMET= '_         '         /PHOTOMETRIC CONDITIONS? (Y/N)
WEATHER = '_         '         /WEATHER CONDITIONS
COMMENTS= '_         '         /
A_NMATCH=                    4 /NUM OF ASTROM STDS MATCHED
AX_RESID=                 0.31 /RMS ASTROM RESIDUALS (PIXELS):
AY_RESID=                 0.19 /<0 MEANS DEFAULT SOLUTION
HISTORY BDR-TYPE ASTROMETRY ADOPTED
END

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