CITPM shape models of asteroid (362) Havnia fitted to a stellar occultation from 7. January 2017. In all the figures, north is up and west is right. The blue solid contour and the magenta dashed contour represent the model for pole 1 and pole 2, respectively. Black lines in those figures mark occultation shadow chords calculated from occultation timings, with timing uncertainties shown at the extremities of each chord. The scale in seconds is given for reference as a red line. Negative (no occultation) chords are marked with dotted lines, while visual observations (as opposed to video or photoelectric) are marked with dashed lines. See Table 3 for diameters of equivalent volume spheres.