Null geodesics of normal and phantom Einstein-Maxwell-dilaton black holes are
determined analytically by the Weierstrass elliptic functions. The black hole
parameters other than the mass enter, with the appropriate signs, the formula
for the angle of deflection to the second order in the inverse of the impact
parameter allowing for the identification of the nature of matter (phantom or
normal). Such identification is also possible via the time delay formula and
observation of relativistic images. Scattering experiencesmay favor black holes
of Einstein-anti-Maxwell-dilatonic theory for their high relative discrepancy
with respect to the Schwarzschild value. For the cases we restrict ourselves
to, phantom black holes are characterized by the absence of many-world and
two-world null geodesics.Comment: 30 pages, 14 figures (with 7 captions), minor correction