All Tables

Table 1: The sample. For each source the number of flares, the number of datapoints since 1980 in each frequency band, the maximum flux density ( $S_{\rm max}$ ), variability index V and median duration of flares at 37 GHz are listed. Column 4 indicates if the source is a high-confidence EGRET detection (x) or a possible detection (?).
Table 2: Median values of duration, observed peak flux density and relative peak flux density for all frequencies and source classes. Number of flares used to calculate the value is also shown.