Acknowledments

This work is supported in part by the National Science Foundation REU and Department of Defense ASSURE programs under NSF Grant no. 1262851 and by the Smithsonian Institution

This publication makes use of molecular line data from the Boston University-FCRAO Galactic Ring Survey (GRS). The GRS is a joint project of Boston University and Five College Radio Astronomy Observatory, funded by the National Science Foundation under grants AST-9800334, AST-0098562, and AST-0100793. This publication also makes use of data from the H2O Southern Galactic Plane Survey and the The Millimetre Astronomy Legacy Team 90 GHz Survey.

This work is based [in part] on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA.

The glue software is developed by the Seamless Astronomy group at the Center for Astrophysics, under contract to NASA’s James Webb Space Telescope program. WorldWide Telescope has been developed and supported by Microsoft Research, in part through gifts to the Seamless Astronomy program, and it will become an open-source resource available on GitHub in 2015.