  We report on a survey of the inner part of the Galactic Plane in very high
energy gamma-rays, with the H.E.S.S. Cherenkov telescope system. The Galactic
Plane between +-30deg in longitude and +-3deg in latitude relative to the
Galactic Centre was observed in 500 pointings for a total of 230 hours,
reaching an average flux sensitivity of 2% of the Crab Nebula at energies above
200 GeV. Fourteen previously unknown sources were detected at a significance
level greater than 4 sigma after accounting for all trials involved in the
search. Initial results on the eight most significant of these sources were
already reported elsewhere. Here we present detailed spectral and morphological
information for all the new sources, along with a discussion on possible
counterparts in other wavelength bands. The distribution in Galactic latitude
of the detected sources appears to be consistent with a scale height in the
Galactic disk for the parent population smaller than 100 pc, consistent with
expectations for supernova remnants and/or pulsar wind nebulae.
