Three-mm Ultimate Mopra Milky Way Survey (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.

ThrUMMS 12CO integrated intensity

ThrUMMS 13CO integrated intensity

Reference

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

Original WCS Data

Project Website

https://users.astro.ufl.edu/~peterb/research/thrumms/