  The first half of the review dedicated to survey works on Be stars (Baade,
Martayan, and Rivinius, this vol.) put emphasis on what we can learn from
surveys about Be stars as a part of an environment, such as Be stars in
binaries, Be stars in different metalicities, or Be stars as part of a star
forming and then co-evolving group. This second half will rather concentrate on
the information that more focused surveys can give on a Be star, understood as
an individual object, and in this way attempts to bridge the gap between highly
detailed single star studies, and necessarily broad survey and catalog work.
