  A high-resolution spectropolarimetric survey of all (573) stars brighter than
magnitude V=4 has been undertaken with Narval at TBL, ESPaDOnS at CFHT, and
HarpsPol at ESO, as a ground-based support to the BRITE constellation of
nano-satellites in the framework of the Ground-Based Observation Team (GBOT).
The goal is to detect magnetic fields in BRITE targets, as well as to provide
one very high-quality, high-resolution spectrum for each star. The survey is
nearly completed and already led to the discovery of 42 new magnetic stars and
the confirmation of several other magnetic detections, including field
discoveries in, e.g., an Am star, two {\delta} Scuti stars, hot evolved stars,
and stars in clusters. Follow-up spectropolarimetric observations of
approximately a dozen of these magnetic stars have already been performed to
characterise their magnetic field configuration and strength in detail.
