We construct the gauge field and graviton propagators in Euclidean AdS(d+1)
space-time by two different methods. In the first method the gauge invaria
nt Maxwell or linearized Ricci operator is applied directly to bitensor ans
atze for the propagators which reflect their gauge structure. This leads to
a rapid determination of the physical part of the propagators in terms of
elementary functions. The second method is a more traditional approach usin
g covariant gauge fixing which leads to a solution for both physical and ga
uge parts of the propagators. The gauge invariant parts agree in both metho
ds. (C) 1999 Elsevier Science B.V. Ail rights reserved.