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ThrUMMS
The Three-mm Ultimate Mopra Milky Way Survey (ThrUMMS) mapped the 12CO(1-0), 13CO(1-0), C18O(1-0), and CN(1-0) emission within the fourth Galactic quadrant using the Mopra Telescope.
ThrUMMS covers a longitude range l = (-60°,0°) and a latitude range of |b| < 1°. The angular resolution of ThrUMMS is ~60 arcseconds and the velocity resolution is 0.3 km/s. The typical rms sensitivity per channel of the ThrUMMS data cubes is σ(T) ~ 2K for 12CO, and ~1K for the other transitions.
CADE currently delivers 12CO(1-0), 13CO(1-0) and C18O(1-0) integrated intensity and peak brightness maps of the full ThrUMMS region using the survey's public DR4.
Please contact us cade@irap.omp.eu if you are interested in HEALPix maps of the CN transitions surveyed by ThrUMMS, or if you require maps at a different angular resolution for your science.
References
- 'The Three-mm Ultimate Mopra Milky Way Survey. I. Survey Overview, Initial Data Releases and First Results', Barnes, P. et al, 2015, ApJ, 812 6
Maps
HiPS
For the corresponding HIPS, unzip the directory and put it directly in an Aladin window to display the map
Known Issues
Version History
- v1 CADE maps, March 2022