COSMOS field Ly{alpha} emitters at z~5.7 (Murayama+, 2007)

Details COSMOS field Ly{alpha} emitters at z~5.7 (Murayama+, 2007) COSMOS field Ly{alpha} emitters at z~5.7 (Murayama+, 2007)

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..21720523m&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/172/523. Originally published in: 2007ApJS..172..523M

Computer Science

Surveys, Redshifts, Equivalent Widths, Photometry: Sdss

Scientific paper

We present results from a narrow-band optical survey of a contiguous area of 1.95deg2, covered by the Cosmic Evolution Survey (COSMOS). Both optical narrow-band ({lambda}c=8150{AA} and {delta}{lambda}=120{AA}) and broad-band (B, V, g', r', i', and z') imaging observations were performed with the Subaru prime-focus camera, Suprime-Cam on the Subaru Telescope. We provide the largest contiguous narrow-band survey, targeting Ly{alpha} emitters (LAEs) at z~5.7. We find a total of 119 LAE candidates at z~5.7. Over the wide-area covered by this survey, we find no strong evidence for large-scale clustering of LAEs. We estimate a star formation rate (SFR) density of ~7×10-4M{sun}/yr/Mpc3 for LAEs at z~5.7 and compare it with previous measurements.
(2 data files).

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