Lyman Alpha Emitters at Redshift 5.7 in the COSMOS Field
arXiv:astro-ph/0702458 · doi:10.1086/516597
Abstract
We present results from a narrow-band optical survey of a contiguous area of 1.95 deg^2, 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, targetting 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^-4 M_sun yr^-1 Mpc^-3 for LAEs at z~5.7, and compare it with previous measurements.
26 pages, 19 figures. to appear in the ApJ Supplement COSMOS Special Issue
References in corpus (5)
- The Cosmic Evolution Survey (COSMOS) -- Overview
- The Cosmic Evolution Survey (COSMOS): Subaru Observations of the HST COSMOS Field
- Rapid Evolution in the Most Luminous Galaxies During the First 900 Million Years
- The Wide Field Imager Lyman-Alpha Search (WFILAS) for Galaxies at Redshift ~5.7: II. Survey Design and Sample Analysis
- Radio and millimeter properties of Ly emitters in the COSMOS field: limits on radio AGN, submm galaxies, and dust obscuration
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- A Magellan M2FS Spectroscopic Survey of Galaxies at 5.5<z<6.8: Program Overview and a Sample of the Brightest Lyman-alpha Emitters
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