Notes. Precise star positions and geocentric Pluto positions for 16 stellar occultation dates between 2005−2013 are listed. The ICRS positions of the stars are given at noon of the occultation date in Col. 1. The mean error refers to the standard deviations of the (O−C)s from the (α, δ) star reductions. The repeatability is the standard deviation of the star position. All star positions were obtained using the UCAC4 as reference star catalog. The number of UCAC4 stars in each frame varies typically between 100 (for Perkin-Elmer) and 500 (for Zeiss and Boller & Chivens), depending on the size of the FOV. The epoch of the observation of the stars are given. The positions were corrected by UCAC4 proper motions, when available, to place the star positions at the occultation epochs given in the table. Proper motions from other catalogs were used otherwise (see text). Magnitudes in the R band were taken from the catalogs that provided the proper motions to the respective stars. The offsets on Pluto’s positions, as obtained from the stellar occultations, are given with respect to DE421 and are in the sense observation minus DE421 (see Fig. 12). The positions of Pluto in the two last columns are geocentric astrometric positions in the ICRS, as obtained from stellar occultations (that is, corrected for the respective offsets). The associated JD is close (about 1s) to the geocentric closest approach. The relative geocentric distance of Pluto with respect to the star is determined with mas accuracy from the fitting of the light curves of stellar occultations. Adding our star positions to these distances allowed us to obtain the listed 16 Pluto positions for these occultations. These Pluto positions are as precise as the positions derived for the stars themselves.