✎ FUGIN [CADE]

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====== 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 [[mailto:cade@irap.omp.eu|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

=== Original WCS Data ===
http://jvo.nao.ac.jp/portal/nobeyama/fugin.do

=== Project Website ===
https://nro-fugin.github.io/

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