  The high-resolution (R = 10^4) near-ultraviolet IUE spectrum of the peculiar
post Asymptotic Giant Branch (post-AGB) supergiant HD101584 (F0Iape) has been
analyzed. In the wavelength range between 2500 and 3000ang, 291 out of 332
absorption features are identified. The main contribution comes from FeII, CrII
and MnII. Most of the absorption features are blends from several absorption
lines. This is mainly due to the intrinsic broad line profiles in the spectrum
of HD101584 in combination with the many absorption lines which occur in the UV
for a F-type spectrum. The list compiled gives for all measured absorption
features between 2500 and 3000ang the measured central wavelength of the core
of the profile, the equivalent width of the profile if this could be
determined, the depth of the profile, an asymmetry factor, a quality factor and
lists the transitions which are responsible for the feature. An analysis of the
radial velocities of the absorption profiles will be give in a separate paper.
