This is an old revision of the document!
FUGIN
The FOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45-m telescope (FUGIN) project was one of the legacy projects utilizing the new multi-beam receiver FOREST (FOur-beam REceiver System on the 45 m Telescope).
FUGIN observed the the 12CO(1-0), 13CO(1-0) and C18O(1-0). molecular line transitions across the longitude ranges l = (+10°,+50°) and l = (+198°,+236°), within a latitude range of |b| < 1°. The total survey area is XXX square degrees.
The intrinsic angular resolution of the FUGIN survey data is ~20 arcseconds, and the velocity resolution is XX km/s. The typical rms sensitivity per XX km/s channel of the FUGIN data cubes is σ(T) ~XXK.
CADE currently delivers 12CO(1-0), 13CO(1-0) and C18O(1-0) integrated intensity and peak brightness maps of the full FUGIN region using the survey's public data release.
Please contact us cade@irap.omp.eu if you require FUGIN maps at a different resolution for your science.
References
- 'FOREST unbiased Galactic plane imaging survey with the Nobeyama 45 m telescope (FUGIN). I. Project overview and initial results', Umemoto, T et al. 2017, PASJ, 69, 78.
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