The following was produced by batchlow1 on Mon Jul  1 12:50:44 2002
    Star: RXJ 2117+3412
           3   Spectra Found
    CAM  IMAGE    APER    MODE    NAME 
    SWP  50917      L      P     RXJ 2117+341  Note see below
    SWP  50918      L      P     RXJ 2117+341
    SWP  50919      L      P     RXJ 2117+341

           3   Unique Image IDs 
SWP50917.MXLO
SWP50918.MXLO
SWP50919.MXLO

                Spectra Written to Output File
Spectrum    Extracted  Multiple   Trailed      Segmented    Exp(s),  MODE
SWP50917L      POINT         NO   NO-TRAIL         NO       599.5    0
SWP50918L      POINT         NO   NO-TRAIL         NO       299.7    0
SWP50919L      POINT         NO   NO-TRAIL         NO       359.5    0
Total of       3 Spectra

RATIO START
SWP50917L : SWP50919L 
SWP50918L : SWP50919L
RATIO STOP

COADD START :3:rxj2117+3412_S.COADD
SWP50917L  000.00  1.000      599.0  1000.0  1000.0
SWP50918L  000.00  1.000      299.0  1212.0  1220.8
SWP50919L  000.00  1.000      359.0  1000.0  1000.0
COADD STOP


Note:  None of the fluxes of these three images agree.
Feibelman, Walter A., 1999ApJ...513..947F lists this
as a flux variable.  The coadded spectrum is the mean.