Notes. Only 45 sources had an adequate decomposition of the total flux density curves at 37 GHz. Columns are as follows: (1) source name; (2) alias; (3) spectroscopic type; (4) the phase of the mm flare at the time of the γ-ray peak (0–1 growing phase, 1–2 decaying phase); (5) the observed time delay between the onset of a mm flare and the γ-ray peak; (6) the linear distance between the region of mm-flare inception (i.e. radio-core) and the location of the γ-ray emission region.