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The advent of the Fermi-GST with its unprecedented capability to monitor theentire 4 pi sky within less than 2-3 hours, introduced new standard in timedomain gamma-ray astronomy. To explore this new avenue of extragalactic physicsthe F-GAMMA programme undertook the task of conducting nearly monthly,broadband radio monitoring of selected blazars from January 2007 to January2015. In this work we release all the light curves at 2.64, 4.85, 8.35, 10.45,14.6, 23.05, 32, and 43 GHz and present first order derivative data productsafter all necessary post-measurement corrections and quality checks; that isflux density moments and spectral indices. The release includes 155 sources.The effective cadence after the quality flagging is around one radio SED every1.3 months. The coherence of each radio SED is around 40 minutes. The releaseddataset includes more than $4\times10^4$ measurements. The median fractionalerror at the lowest frequencies (2.64-10.45 GHz) is below 2%. At the highestfrequencies (14.6-43 GHz) with limiting factor of the atmospheric conditions,the errors range from 3% to 9%, respectively.

F-GAMMA: Multi-frequency radio monitoring of Fermi blazars. The 2.64 to 43 GHz Effelsberg light curves from 2007-2015