We identified microsaccades automatically with an objective algorithm (for details, see Engbert & Kliegl,
2003b). To reduce the amount of potential noise (Engbert,
2006), we considered only binocular microsaccades, that is, microsaccades with a minimum overlap of one data sample in both eyes (Engbert,
2006; Engbert & Mergenthaler,
2006; Laubrock, Engbert, & Kliegl,
2005; Rolfs et al.,
2006). Additionally, we imposed a minimum intersaccadic interval of 20 ms so that potential overshoot corrections might not be categorized as new microsaccades (Møller, Laursen, Tygesen, & Sjølie,
2002). The microsaccadic main sequence is plotted in
Figures 1C and
1D.
Figure 1C shows the peak velocity–magnitude relationship for all microsaccades (
n = 16,956 microsaccades; Zuber & Stark,
1965), and
Figure 1D shows their duration-magnitude relationship (Evinger, Shaw, Peck, Manning, & Baker,
1984; Gruart, Blázquez, & Delgado-Garcia,
1995).
Figure 1E plots the distribution of microsaccade magnitudes (up to 3 deg; Engbert & Kliegl,
2003b). Of these, only microsaccades smaller than 1 deg (
n = 16,252 microsaccades) were studied further (Rolfs et al.,
2006) (equivalent results were obtained when using 2- or 3-deg thresholds; data not shown).
Table 1 summarizes various microsaccade parameters for individual subjects and for the subject average.