 18O     18F EC DECAY (1.82890 H)                                               
 18O   H TYP=UPD$AUT=N.K.KUZMENKO$CUT=01-JUN-2014$                              
 18O 2 H TYP=UPD$AUT=V.CHISTE, M.-M.BE$CUT=01-JUN-2006$                         
 18O 3 H TYP=FUL$AUT=V.CHISTE, M.-M.BE$CUT=01-OCT-2002$                         
 18O  C  References:1938Br01, 1943Hu02, 1949Bl26, 1951Ru24, 1956Dr38, 1958Be74, 
 18O 2C  1958Ma68, 1959Aj76, 1959Ca01, 1960Yu02, 1961Ra06, 1962Ma48, 1963Be47,  
 18O 3C  1964Ho28, 1964Ho09, 1964Ma12, 1965Eb01, 1965Bo42, 1970Al11, 1972Aj02,  
 18O 4C  1973Ho43, 1977Ba48, 1978Aj03, 1980RuZY, 1987Aj02, 1989Sc17, 2002Un02,  
 18O 5C  2004BeZQ, 2004Sc04, 2010Ga04, 2012Ha35, 2012Wa38, 2014Un01             
 18O  T  Auger electrons and X ray energies and emission intensities:           
 18O  T       {U Energy (keV)}   {U Intensity}  {U Line}                        
 18O  T                                                                         
 18O  T        0.525              0.007    2     XKA2                           
 18O  T        0.525              0.013    4     XKA1                           
 18O  T                                                                         
 18O  T                                                                         
 18O  T                                                                         
 18O  T                                                                         
 18O  T        0.456-0.502         |] 2.89   2.89    18         KLL AUGER                                       
 18O  T        0.0143           0.229   21     L AUGER                        
 18F   P 0.0         1+                1.82890 H 23             1655.9    5     
 18O   N 1.0         1.0       1         1.0                                    
 18O   L 0           0+                 STABLE                                  
 18O   E             96.86   193.14    193.57                                   
 18O 2 E EAV=249.5     3$CK=0.02911  16$CL=0.00229  16                          
                                                                                
