Near-Infrared Properties of I-Drop Galaxies in the Hubble Ultra Deep   Field
  We analyse near-infrared HST/NICMOS F110W (J) and F160W (H) band photometry of a sample of 27 i'-drop candidate z~6 galaxies in the central region of the HST/ACS Ultra Deep Field (HUDF). The infrared colours of the 20 objects not affected by near neighbours are consistent with a high redshift interpretation. This suggests that the low redshift contamination of this i'-drop sample is smaller than that observed at brighter magnitudes where values of 10-40% have been reported. The J-H colours are consistent with a slope flat in f_nu (f_lam \propto lam^{-2}), as would be expected for an unreddened starburst. There is, however, evidence for a marginally bluer spectral slope (f_lam propto lam^{-2.2) which is perhaps indicative of an extremely young starburst (~10 Myr old) or a top heavy initial mass function and little dust. The low levels of contamination, median photometric redshift of z~6.0 and blue spectral slope, inferred using the near-infrared data, supports the validity of the assumptions in our earlier work in estimating the star formation rates and, that the majority of the i-drop candidates galaxies lie at z~6. 
Elizabeth Stanway (IOA, Cambridge), Richard McMahon (IOA, Cambridge),   Andrew Bunker (IOA, Cambridge & Exeter)