Fig. 2

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Map of post-occultation shadow path of the stellar occultation by Huya, the path width (limited by the blue lines) is the area-equivalent diameter obtained from the reconstructed ellipse fit (D = 411.3 km, see Sect. 5.1). The site positions from where the occultation was recorded are shown with green marks, the negative detections with red marks, and the sites that did not observe due to bad weather or to technical problems are indicated with white marks. The green line indicates the centrality of the shadow path and the blue lines the limits of the shadow. The arrow in the right bottom shows the direction of the shadow motion3.
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