A LUMINOUS Lyα-EMITTING GALAXY AT REDSHIFT z = 6.535: DISCOVERY AND SPECTROSCOPIC CONFIRMATION

摘要

We present a redshift z = 6.535 galaxy discovered by its Lyα emission in a 9180 A narrowband image from the Large Area Lyman Alpha survey. The Lyα line luminosity (1.1 x 10~(43) ergs s~(-1)) is among the largest known for star-forming galaxies at z ≈ 6.5. The line shows the distinct asymmetry that is characteristic of high-redshift Lyα. The 2 σ lower bound on the observer-frame equivalent width is greater than 530 A. This is hard to reconcile with a neutral intergalactic medium (IGM) unless the Lyα line is intrinsically strong and is emitted from its host galaxy with an intrinsic Doppler shift of several hundred km s~(-1). If the IGM is ionized, it corresponds to a rest-frame equivalent width greater than 40 A after correcting for Ly? forest absorption. We also present a complete spectroscopic follow-up of the remaining candidates with line flux greater than 2 x 10~(-17) ergs cm~(-2) s~(-1) in our 1200 arcmin~2 narrowband image. These include another galaxy with a strong emission line at 9136 A and no detected continuum flux, which, however, is most likely an [O Ⅲ] λ5007 source at z = 0.824, on the basis of a weak detection of the [O Ⅲ] λ4959 line.