Notes. Occultation table: day of the year and UTC time of the prediction; right ascension and declination of the occulted star – in the original table, these coordinates are immediately followed by the geocentric astrometric equatorial coordinates (corrected for the offset or ephemeris method), not presented here, of the occulting body; C/A: the geocentric closest approach, in arcseconds; P/A: the planet position angle with respect to the occulted star at C/A, in degrees; velocity in plane of sky, in km s^-1: positive = prograde, negative = retrograde; D: planet range to Earth, in AU; R*, J*, H*, K*: normalized magnitudes to a common shadow velocity of 20 km s^-1 by the relationship Mag* = Mag. A value of 50.0 means that the star is not in the 2MASS; λ: east longitude of subplanet point in degrees, positive towards east; LST: UT + λ: local solar time at subplanet point, hh:mm; Δe_α ∗ and Δe_δ: offset in mas applied to the ephemeris right ascension and declination, respectively; pm: ok = proper motion applied, no = no proper motion applied; catalogue cross-identification (ct) = uc (UCAC2), 2 m (2MASS), fs (field star); f = multiplicity flag (see Table 3); E_α ∗ and E_δ: uncertainties (mas) in right ascension and declination. A value of 9999 means that there was no estimation of the respective uncertainty; μ_α ∗ and μ_δ: proper motions in right ascension and declination, respectively (mas/year).