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Table 8

CDS data table sample for Himalia.

RA (ICRS) Dec RA error Dec error Epoch Mag Filter Telescope IAU code
h m s ° ′ ″ (mas) (mas) (jd)
16 59 11.6508 –22 00 44.855 17 12 2 454 147.78241319 16.0 C BC 874
16 59 11.6845 –22 00 44.932 17 12 2 454 147.78332384 15.8 C BC 874
16 59 11.7181 –22 00 44.978 17 12 2 454 147.78422477 16.0 C BC 874
16 59 11.7818 –22 00 45.143 17 12 2 454 147.78602662 15.9 C BC 874
16 59 11.8188 –22 00 45.232 17 12 2 454 147.78693750 16.0 C BC 874
17 17 11.0344 –22 47 19.415 30 24 2 454 205.63885463 16.1 U BC 874
17 17 11.0270 –22 47 19.381 30 24 2 454 205.63959167 16.1 U BC 874
17 17 11.0258 –22 47 19.366 30 24 2 454 205.64031875 16.1 U BC 874
17 17 11.0192 –22 47 19.417 30 24 2 454 205.64104583 16.1 U BC 874

Notes. This sample corresponds to 9 observations of Himalia from February 16, 2007 and April 15, 2007. Tables contain the topocentric ICRS coordinates of the irregular satellites, the position error estimated from the dispersion of the ephemeris offsets of the night of observation, the UTC time of the frame’s mid-exposure in Julian date, the estimated magnitude, the filter used, the telescope origin and correspondent IAU code. The filters may be U, B, V, R or I following the Johnson system; C stands for clear (no filter used), resulting in a broader R-band magnitude, RE for the broad-band R filter ESO#844 with λc = 651.725 nm and Δλ = 162.184 nm (full width at half maximum) and “un” for unknown filter. E, OH, PE, BC and Z stand for the ESO, OHP, Perkin-Elmer, Bollen & Chivens, and Zeiss telescopes, respectively.

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