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arXiv · 1808.02533

The Radio Ammonia Mid-Plane Survey (RAMPS) Pilot Survey

Taylor Hogge·James Jackson·Ian Stephens·Scott Whitaker·Jonathan Foster·Matthew Camarata·D. Anish Roshi·James Di Francesco·Steven Longmore·Robert Loughnane·Toby Moore·Jill Rathborne·Patricio Sanhueza·Andrew Walsh
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Abstract

The Radio Ammonia Mid-Plane Survey (RAMPS) is a molecular line survey that aims to map a portion of the Galactic midplane in the first quadrant of the Galaxy (l = 10 deg - 40 deg, |b| < 0.4 deg) using the Green Bank Telescope. We present results from the pilot survey, which has mapped approximately 6.5 square degrees in fields centered at l = 10 deg, 23 deg, 24 deg, 28 deg, 29 deg, 30 deg, 31 deg, 38 deg, 45 deg, and 47 deg. RAMPS observes the NH3 inversion transitions NH3(1, 1) - (5, 5), the H2O 6(1,6) - 5(2,3) maser line at 22.235 GHz, and several other molecular lines. We present a representative portion of the data from the pilot survey, including NH3(1,1) and NH3(2,2) integrated intensity maps, H2O maser positions, maps of NH3 velocity, NH3 line width, total NH3 column density, and NH3 rotational temperature. These data and the data cubes from which they were produced are publicly available on the RAMPS website (http://sites.bu.edu/ramps/).

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Taylor Hogge, James Jackson, Ian Stephens, Scott Whitaker, Jonathan Foster, Matthew Camarata, D. Anish Roshi, James Di Francesco, Steven Longmore, Robert Loughnane, Toby Moore, Jill Rathborne, Patricio Sanhueza, Andrew Walsh. 2018-08-07. The Radio Ammonia Mid-Plane Survey (RAMPS) Pilot Survey. https://doi.org/10.3847/1538-4365/aacf94

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