Bright Lyα emitters at z ∼ 9: constraints on the LF from HizELS

New results are presented, as part of the Hi-z Emission Line Survey (HizELS), from the largest area survey to date (1.4 deg(2)) for Ly alpha emitters (LAEs) at z similar to 9. The survey, which is primarily targeting Ha emitters at z < 3, uses the Wide Field CAMera on the United Kingdom Infrared Telescope and a custom narrow-band filter in the J band and reaches a Ly alpha luminosity limit of similar to 10(43.8) erg s(-1) over a co-moving volume of 1.12 x 10(6) Mpc(3) at z = 8.96 +/- 0.06. Only two candidates were found out of 1517 line emitters and those were rejected as LAEs after follow-up observations. The limit on the space density of bright LAEs is improved by three orders of magnitude, consistent with suppression of the bright end of the Ly alpha luminosity function beyond z similar to 6. Combined with upper limits from smaller but deeper surveys, this rules out some of the most extreme models for high-redshift LAEs. The potential contamination of future narrow-band Ly alpha surveys at z > 7 by Galactic brown dwarf stars is also examined, leading to the conclusion that such contamination may well be significant for searches at 7.7 < z < 8.0, 9.1 < z < 9.5 and 11.7 < z < 12.2.