Vicki Lowe

The H2O Southern Galactic Plane Survey: NH3 (1,1) and (2,2) catalogues

The H₂O Southern Galactic Plane Survey (HOPS) has mapped a 100 degrees strip of the Galactic plane (-70° > l > 30°, |b| 10⁴cm⁻³). In this paper, we present the NH₃ (1,1) and (2,2) data, which have a resolution of 2 arcmin and cover a velocity range of ± 200 km s⁻¹. The median sensitivity of the NH₃ data cubes is σT(mb) =0.20 ± 0.06 K. For the (1,1) transition, this sensitivity equates to a 3.2 kpc distance limit for detecting a 20 K, 400 M⊙ cloud at the 5σ level. Similar clouds of mass 5000 M⊙ would be detected as far as the Galactic Centre, while 30000 M⊙ clouds would be seen across the Galaxy. We have developed an automatic emission finding procedure based on the Australian Telescope National Facility (ATNF) duchamp software and have used it to create a new catalogue of 669 dense molecular clouds. The catalogue is 100 per cent complete at the 5s detection limit (T(mb) = 1.0 K). A preliminary analysis of the ensemble cloud properties suggests that the near-kinematic distances are favoured. The cloud positions are consistent with current models of the Galaxy containing a long bar. Combined with other Galactic plane surveys this new molecular-line data set constitutes a key tool for examining Galactic structure and evolution. Data cubes, spectra and catalogues are available to the community via the HOPS website.

THE THREE-MM ULTIMATE MOPRA MILKY WAY SURVEY. I. SURVEY OVERVIEW, INITIAL DATA RELEASES, AND FIRST RESULTS

We describe a new mm-wave molecular-line mapping survey of the southern Galactic Plane and its first data releases. The Three-mm Ultimate Mopra Milky Way Survey (ThrUMMS) maps a 60{\deg}x2{\deg} sector of our Galaxys fourth quadrant, using a combination of fast mapping techniques with the Mopra radio telescope, simultaneously in the J=1-0 lines of

MALT-45: a 7 mm survey of the southern Galaxy - I. Techniques and spectral line data

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Maser Source-Finding Methods in HOPS

CO,

Accurate OH maser positions from the SPLASH pilot region

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TRACING H2 COLUMN DENSITY WITH ATOMIC CARBON (C I) AND CO ISOTOPOLOGS

CO, C

Pilot observations for MALT-45: a Galactic plane survey at 7 mm

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Molecular line mapping of the giant molecular cloud associated with RCW 106 - IV. Ammonia towards dust emission

O, and CN near 112 GHz at ~arcminute and ~0.3 km s

Ammonia towards dust clumps in the giant molecular cloud associated with RCW 106

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A 3-mm molecular line study of the Central Molecular Zone of the Galaxy

resolution, with ~2 K channel