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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 1 arcminute 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) and 13CO(1-0) integrated intensity and peak brightness maps of the full ThrUMMS region using the survey's public DR4.
Healpix maps made by A. Hughes.
Reference
- '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 https://ui.adsabs.harvard.edu/abs/2015ApJ...812....6B
| 12CO TPK | 13CO TPK |
|---|---|
Maps
12CO Integrated Intensity : THRUMMS_12CO_MOM0_1_8192_partial.fits
12CO Peak Brightness : THRUMMS_12CO_TPK_1_8192_partial.fits
13CO Integrated Intensity : THRUMMS_13CO_MOM0_1_8192_partial.fits
13CO Peak Brightness : THRUMMS_13CO_TPK_1_8192_partial.fits
HiPS
Enter the following URLs in Aladin (“Files” then “Use directly a URL”):
http://cade.irap.omp.eu/documents/Ancillary/4Aladin/THRUMMS_12CO_TPK
http://cade.irap.omp.eu/documents/Ancillary/4Aladin/THRUMMS_13CO_TPK
Known Issues
Version History
- v1 CADE maps, March 2022*/