Extended Data Figure 2 : Map of Earth showing the locations of the observatories that recorded the occultation (green dots).
From: The size, shape, density and ring of the dwarf planet Haumea from a stellar occultation

The solid lines mark the limits of the shadow path. Mount Agliale is indicated in blue because the occultation by the main body was not positive there, but the occultation by the ring was detected. The dashed line denotes the centre of the shadow path. Note that Munich corresponds to the location of the Bavarian Public Observatory. The complete names of the observatories can be found in Table 1. The red marks at Trebur and Valle D’Aosta observatories indicate the two closest sites to the shadow path that recorded a negative occultation. The coordinates of Trebur observatory are 49° 55′ 31.5″ N, 8° 24′ 40.6″ E and the coordinates of Valle D’Aosta observatory are 45° 47′ 22″ N and 7° 28′ 42″ E. The shadow motion is from the bottom to the top of the figure.