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  1. SIMPLE  =                    T /CONFORMS TO FITS FORMAT?                        BITPIX  =                   16 /NUMBER OF BITS PER PIXEL                        NAXIS   =                    1 /NUMBER OF AXES IN ARRAY                         NAXIS1  =                 1291 /DIMENSION OF FASTEST VARYING AXIS               EXTEND  =                    T                                                  OBJECT  = 'VB106 G5V SOLAR ANALOG                                              'FILE-NUM=               700005 /NUMBER OF FILE SENT FROM SPECTRSCPY TO JPL      DATE-OBS= '20/02/84          ' /DATE OF MIDDLE OF DATA ACQUISITION              TIME-OBS=              0.09090 /FRACTION OF DATE                                DATE-REL= '01/04/85          ' /RELEASE DATE                                    DISCIPLN= 'SPECTROSCOPY      ' /IHW DISCIPLIN                                   LONG-OBS= '248/27/51         ' /LONGITUDE OF STATION                            LAT--OBS= '+35/05/49         ' /LATITUDE OF STATION                             SYSTEM  = '76880101          ' /STATION SYSTEM CODE                             OBSERVER= 'LUTZ,B/WAGNER,M                                                     'SUBMITTR= 'WAGNER,M                                                            'SPEC-EVT=                    F /SPECIAL EVENT FLAG                              DAT-FORM= 'STANDARD'           /DATA FORM                                       DAT-TYPE= 'REDUCED DIGITAL   ' /DATA TYPE                                       DIS-CODE= '010106052         ' /DISCIPLIN CODE                                  OBSVTORY= 'LOWELL OBSERVATORY                                                  'TELESCOP= '1.8-M                                                               'INSTRUME= 'Y SPECT/IDS/600GPM                                                  'ELEV-OBS=                 2130 /STATION ELEVATON (METERS)                       RESOL-SP= '9                 ' /APPROX. SPECTRAL RESOLUTION (ANG.)              RANGE-SP= '3820-6400         ' /APPROX. SPECTRAL RANGE (ANG.)                   EXPOSURE=           1920.00000 /EXPOSURE-INTEGRATION TIME (SECONDS)             APERSIZE= '7.46              ' /APER SIZE OR SLIT WIDTH & LEN.(ARCSECS)         QUALITY = 'VERY GOOD         ' /QUALITY FLAG (1-6)                              CTYPE1  = 'LAMBDA            ' /UNITS OF INDEPENDENT VARIABLE                   BUNIT   = 'FLAMBDA           ' /UNITS OF DEPENDENT VARIABLE                     CRVAL1  =         0.382000E+04 /REFERENCE POINT VALUE FOR CTYPE1                CRPIX1  =         0.100000E+01 /REFERENCE PIXEL FOR CTYPE1                      CDELT1  =         0.200000E+01 /INCREMENT IN CTYPE1 PER PIXEL                   HISTORY   DATE-CMP 16/06/85                                                     COMMENT     HARDORP SOLAR ANALOG                                                BSCALE  =         0.358475E-16 /SCALE FACTOR FOR PIXEL TO TRUE VALUES           BZERO   =         0.194890E-11 /OFFSET APPLIED TO TRUE PIXEL VALUES             DEP-MAX =         0.312352E-11 /MAXIMUM OF DEPENDENT VARIABLE                   DEP-MIN =         0.774253E-12 /MINIMUM OF DEPENDENT VARIABLE                   END                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                     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