SPECTROSCOPIC CONFIRMATION OF A z = 6.740 GALAXY BEHIND THE BULLET CLUSTER*

We present the first results of our spectroscopic follow-up of 6.5 5? significance using a 16 hr long exposure with FORS2 VLT. Based on the absence of flux in bluer broadband filters, the blue color of the source, and the absence of additional lines, we identify the line as Ly? at z = 6.740 ? 0.003. The integrated line flux is f = (0.7 ? 0.1 ? 0.3) ? 10?17 erg?1 s?1 cm?2 (the uncertainties are due to random and flux calibration errors, respectively) making it the faintest Ly? flux detected at these redshifts. Given the magnification of ? = 3.0 ? 0.2 the intrinsic (corrected for lensing) flux is f int = (0.23 ? 0.03 ? 0.10 ? 0.02) ? 10?17 erg?1 s?1 cm?2 (additional uncertainty due to magnification), which is ~2-3 times fainter than other such measurements in z ~ 7?galaxies. The intrinsic H 160W-band magnitude of the object is , corresponding to 0.5 L* for LBGs at these redshifts. The galaxy is one of the two sub-L* LBG galaxies spectroscopically confirmed at these high redshifts (the other is also a lensed z = 7.045 galaxy), making it a valuable probe for the neutral hydrogen fraction in the early universe.