The Radio Ammonia Midplane Survey (RAMPS) is a program to survey 60 sq. deg. of the Galactic Plane at 1.3 cm using the Green Bank Telescope. Currently in pilot mode (March 2016), the program will map from l=10° - 40° and b= -0.5° - 0.5°. The RAMPS survey is a successor to the HOPS survey and will cover multiple ammonia transitions at higher resolution and sensitivity than its predecessor. The main science goal of RAMPS includes characterizing the Galactic population of dense star forming gas through a systematic analysis of its properties (e.g. column densities, radial velocities, gas temperatures). The link to the homepage of the RAMPS survey can be found here.
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RAMPS Extended Observations: Spectral Line (3D)
Sep 5, 2016
James Jackson, 2016, "RAMPS Extended Observations: Spectral Line (3D)", https://doi.org/10.7910/DVN/NMDU7W, Harvard Dataverse, V1
This dataset consists of extended spectral line observations taken with the K-band Focal Plane Array on the Green Bank Telescope (GBT). Lines of study include NH3 (1,1); (2,2); (3,3); (4,4); (5,5), H2O masers, and CH3OH masers. This is a blind survey covering 10° < l < 40° and b < |0.5°|. As of summer 2016, no data has been released; however, once...
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