The RMS Survey: H2O masers towards a sample of southern hemisphere
  massive YSO candidates and ultra compact HII regions
  Context: The Red MSX Source (RMS) survey has identified a large sample of
candidate massive young stellar objects (MYSOs) and ultra compact (UC) HII
regions from a sample of ~2000 MSX and 2MASS colour selected sources. Aims: To
search for H2O masers towards a large sample of young high mass stars and to
investigate the statistical correlation of H2O masers with the earliest stages
of massive star formation. Methods: We have used the Mopra Radio telescope to
make position-switched observations towards ~500 UCHII regions and MYSOs
candidates identified from the RMS survey and located between 190\degr < l <
30\degr. These observations have a 4$\sigma$ sensitivity of ~1 Jy and a
velocity resolution of ~0.4 km/s.} Results: We have detected 163 H2O masers,
approximately 75% of which were previously unknown. Comparing the maser
velocities with the velocities of the RMS sources, determined from 13CO
observations, we have identified 135 RMS-H2O maser associations, which
corresponds to a detection rate of ~27%. Taking into account the differences in
sensitivity and source selection we find our detection rate is in general
agreement with previously reported surveys. Conclusions: We find similar
detection rates for UCHII regions and MYSOs candidates, suggesting that the
conditions needed for maser activity are equally likely in these two stages of
the star formation process. Looking at the detection rate as a function of
distance from the Galactic centre we find it significantly enhanced within the
solar circle, peaking at ~37% between 6-7 kpc, which is consistent with
previous surveys of UC HII regions, possibly indicating the presence of a high
proportion of more luminous YSOs and HII regions.
