========================================================================== J/PASJ/58/313 Lyalpha emitters in the SUBARU Deep Field (Shimasaku+, 2006) The following files can be converted to FITS (extension .fit .fgz or .fiZ) table1.dat table3.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/PASJ/58/313 ==========================================================================
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Beginning of ReadMe : J/PASJ/58/313 Lyalpha emitters in the SUBARU Deep Field (Shimasaku+, 2006) ================================================================================ Ly-alpha emitters at z = 5.7 in the Subaru deep field. Shimasaku K., Kashikawa N., Doi M., Ly C., Malkan M.A., Matsuda Y., Ouchi M., Hayashino T., Iye M., Motohara K., Murayama T., Nagao T., Ohta K., Okamura S., Sasaki T., Shioya Y., Taniguchi Y. <Publ. Astron. Soc. Jap., 58, 313-334 (2006)> =2006PASJ...58..313S ================================================================================ ADC_Keywords: Surveys ; Photometry ; Redshifts ; Equivalent widths Keywords: galaxies: evolution - galaxies: high-redshift - galaxies: luminosity function, mass function - galaxies: photometry Abstract: We present the properties of Lyalpha emitters (LAEs) at z=5.7 in the Subaru Deep Field. A photometric sample of 89 LAE candidates was constructed from narrow-band data down to NB816=26.0 (AB) in a continuous 725arcmin^2^ area. Spectra of 39 objects satisfying the photometric selection criteria for LAEs were obtained with Subaru and Keck II Telescopes, among which 28 were confirmed LAEs, one was a nearby galaxy, and eight were unclassified. We also obtained spectra of another 24 NB816-excess objects in the field, identifying six additional LAEs. Description: We made spectroscopic observations of 63 objects selected from the NB816-detected catalog with FOCAS on the Subaru Telescope and DEIMOS on the Keck II Telescope. A total of 39 objects were observed with FOCAS in 2002 and 2004 in the multi-slit mode. Twenty-four objects among the 63 were observed with DEIMOS on UT 2004 April 23 and 24.