The Boston University–five College Radio Astronomy Observatory Galactic Ring Survey

The Boston University-Five College Radio Astronomy Observatory Galactic Ring Survey is a new survey of Galactic CO J = 1 → 0 emission. The survey used the SEQUOIA multi pixel array on the Five College Radio Astronomy Observatory 14 m telescope to cover a longitude range of l = 18– 55.7 and a latitude range of |b| < 1, a total of 75.4 square degrees. Using both position-switching and On-The-Fly mapping modes, we achieved an angular sampling of 22, better than half of the telescope’s 46 angular resolution. The survey’s velocity coverage is −5 to 135 km s for Galactic longitudes l ≤ 40 and −5 to 85 km s for Galactic longitudes l > 40. At the velocity resolution of 0.21 km s, the typical rms sensitivity is σ(T A ) ∼ 0.13K. The survey comprises a total of 1,993,522 spectra. We show integrated intensity images (zeroth moment maps), channel maps, position-velocity diagrams, and an average spectrum of the completed survey dataset. We also discuss the telescope and instrumental parameters, the observing modes, the data reduction processes, and the emission and noise characteristics of the dataset. The Galactic Ring Survey data are available to the community at www.bu.edu/galacticring or in DVD form by request. Subject headings: surveys–ISM: clouds–ISM: molecules–Galaxy: kinematics and dynamics–radio lines: general