The Mopra Southern Galactic Plane CO Survey - Data Release 1

Abstract

We present observations of the first ten degrees of longitude in the Mopra carbon monoxide (CO) survey of the southern Galactic plane (Burton et al. 2013), covering Galactic longitude l = 320-330° and latitude b = $\pm$0.5°, and l = 327-330°, b = +0.5-1.0°. These data have been taken at 35 arc sec spatial resolution and 0.1 km/s spectral resolution, providing an unprecedented view of the molecular clouds and gas of the southern Galactic plane in the 109-115 GHz J = 1-0 transitions of 12CO, 13CO, C18O and C17O. Together with information about the noise statistics from the Mopra telescope, these data can be retrieved from the Mopra CO website and the CSIRO-ATNF data archive.

15 pages, 15 figures, accepted by PASA

References in corpus (4)

• The Boston University-Five College Radio Astronomy Observatory Galactic Ring Survey
• Bias-free Measurement of Giant Molecular Cloud Properties
• Milky Way Kinematics: Measurements at the Subcentral Point of the Fourth Quadrant
• Discovery of Luminous Star Formation in PMN1452-5910/IRAS14482-5857: the Pterodactyl Nebula

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• The Steady-State Multi-TeV Diffuse Gamma-Ray Emission Predicted with GALPROP and Prospects for the Cherenkov Telescope Array
• Element Stratification in the Middle-Aged Type Ia Supernova Remnant G344.7-0.1
• A study of the interstellar medium towards the unidentified dark TeV $\gamma$-ray sources HESS J1614-518 and HESS J1616-508
• The G332 molecular cloud ring: I. Morphology and physical characteristics
• Triggered high-mass star formation in the HII region W28A2: A cloud-cloud collision scenario
• Massive star formation in the Carina nebula complex and Gum 31 -- II. a cloud-cloud collision in Gum 31