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The Galactic Center Ridge has been observed extensively in the past by bothGeV and TeV gamma-ray instruments revealing a wealth of structure, including adiffuse component as well as the point sources G0.9+0.1 (a composite supernovaremnant) and Sgr A* (believed to be associated with the supermassive black holelocated at the center of our Galaxy). Previous very high energy (VHE) gamma-rayobservations with the H.E.S.S. experiment have also detected an extended TeVgamma-ray component along the Galactic plane in the >300 GeV gamma-ray regime.Here we report on observations of the Galactic Center Ridge from 2010-2014 bythe VERITAS telescope array in the >2 TeV energy range. From these observationswe 1.) provide improved measurements of the differential energy spectrum forSgr A* in the >2 TeV gamma-ray regime, 2.) provide a detection in the >2 TeVgamma-ray emission from the composite SNR G0.9+0.1 and an improveddetermination of its multi-TeV gamma-ray energy spectrum, 3.) report on thedetection of VER J1746-289, a localized enhancement of >2 TeV gamma-rayemission along the Galactic plane.

TeV Gamma-ray Observations of The Galactic Center Ridge By VERITAS