Abstract
The MIV and MV edges of Gd64, Dy66, and Yb70 were measured using a high-intensity-focusing x-ray spectrograph operating in vacuum. An absorption line is detected on the long-wavelength side of the MIV edge of Gd64 and a weaker one at the MV edge of Dy66. For Yb70, however, the MV absorption has the appearance of a strong "white line." No absorption line has been observed at the MV edge of Gd64 nor at the MIV edges of Dy66 and Yb70. The significance of the occurrence and absence of absorption lines in the filling of the 4f shell of the "heavy" rare earths and the effect of the absorber thickness on the shape of the absorption profile are discussed.