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A group of 72 members of the astrochemistry and spectroscopy communitiesassembled at Emory University in October, 2012, to discuss the state-of-the artin molecular laboratory spectroscopic techniques used to study molecules ofastrophysical interest, and highlight recent successes in laboratory effortsthat complement new astronomical observations. The format of the meetingfacilitated detailed discussion of the needs for collecting and interpretingmolecular spectroscopic information to support observational astrophysics inthe era of Far-IR astronomy. We present the findings and recommendations fromthis workshop in this report. The participants in this workshop identified thedevelopment of new laboratory capabilities that offer rapid, broadband,high-resolution, high-sensitivity measurements of molecular spectra in thefrequency ranges that overlap with new observational facilities as the toppriority for far-infrared laboratory astrophysics initiatives over the next5-10 years. An additional major need is the development of suitable analysistools for broadband molecular spectra from both the laboratory and space;though such efforts should be conducted within the framework of largercollaborative funding structures, rather than through single-PI efforts, so asto provide tools that are generally applicable rather than highly specialized.Additional efforts in theory, computation, and modeling that support thesegoals are also important for advancing this field.

Report from the Workshop on Molecular Spectroscopy in the Era of Far-Infrared Astronomy