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thrumms [2022/02/21 15:35]
ahughes
thrumms [2023/09/22 10:01] (current)
Déborah Paradis
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-====== ThrUMMS ======+====== ​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. 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.+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)13CO(1-0) and C18O(1-0) integrated intensity and peak brightness maps of the full ThrUMMS region using the survey'​s public DR4. +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.
  
 /* /*
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 */ */
  
-Please contact us [[mailto:​cade@irap.omp.eu|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.+/*Please contact us [[mailto:​cade@irap.omp.eu|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 ​=== +=== 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+  * 'The Three-mm Ultimate Mopra Milky Way Survey. I. Survey Overview, Initial Data Releases and First Results',​ Barnes, P. et al, 2015, ApJ, 812https://​ui.adsabs.harvard.edu/​abs/​2015ApJ...812....6B
  
 === Maps === === Maps ===
  
 +12CO Integrated Intensity : [[http://​cade.irap.omp.eu/​documents/​Ancillary/​THRUMMS/​THRUMMS_12CO_MOM0_1_8192_partial.fits|THRUMMS_12CO_MOM0_1_8192_partial.fits]]
  
-===HiPS ===+12CO Peak Brightness : [[http://​cade.irap.omp.eu/​documents/​Ancillary/​THRUMMS/​THRUMMS_12CO_TPK_1_8192_partial.fits|THRUMMS_12CO_TPK_1_8192_partial.fits]]
  
-For the corresponding HIPS, unzip the directory and put it directly in an Aladin window to display the map+13CO Integrated Intensity : [[http://​cade.irap.omp.eu/​documents/​Ancillary/​THRUMMS/​THRUMMS_13CO_MOM0_1_8192_partial.fits|THRUMMS_13CO_MOM0_1_8192_partial.fits]]
  
 +13CO Peak Brightness : [[http://​cade.irap.omp.eu/​documents/​Ancillary/​THRUMMS/​THRUMMS_13CO_TPK_1_8192_partial.fits|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 === === Known Issues ===
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 === Version History === === Version History ===
-  * v1 CADE maps, March 2022+  * v1 CADE maps, March 2022*/
  
 === Original WCS Data === === Original WCS Data ===