Examples of circularly polarized, bandpass-averaged flares from TVLM 513 observed at 4.85 GHz with the Arecibo radio telescope in 2012 and 2013, and phased up according to the best-fit timing model discussed in the text. The vertical, dashed line marks the phase of flare arrival times predicted by the model. For display purposes, the original flare time resolution of 0.9 s has been smoothed to 4.5 s.