  The cosmological constant Lambda affects cosmological gravitational lensing.
Effects due to Lambda can be studied in the framework of the Schwarzschild-de
Sitter spacetime. Two novel contributions, which can not be accounted for by a
proper use of angular diameter distances, are derived. First, a term 2m b
Lambda/3 has to be added to the bending angle, where "m" is the lens mass and
"b" the impact parameter. Second, Lambda brings about a difference in the
redshifts of multiple images. Both effects are quite small for real
astrophysical systems (contribution to the bending < 0.1 microarcsec and
difference in redshift < 10^{-7}).
