  We report the results of a globally coordinated photometric campaign to
search for transits by the P ~ 30 d and P ~ 60 d outer planets of the 3-planet
system orbiting the nearby M-dwarf Gl 876. These two planets experience strong
mutual perturbations, which necessitate use of a dynamical (four-body) model to
compute transit ephemerides for the system. Our photometric data have been
collected from published archival sources, as well as from our photometric
campaigns that were targeted to specific transit predictions. Our analysis
indicates that transits by planet "c" (P ~ 30 d) do not currently occur, in
concordance with the best-fit i = 50 degree co-planar configuration obtained by
dynamical fits to the most recent radial velocity data for the system. Transits
by planet "b" (P ~ 60 d) are not entirely ruled out by our observations, but
our data indicate that it is very unlikely that they occur. Our experience with
the Gl 876 system suggests that a distributed ground-based network of small
telescopes can be used to search for transits of very low mass M-stars by
terrestrial-sized planets.
