The Wide Field Imager Lyman-Alpha Search (WFILAS) for Galaxies at Redshift ~5.7: I. A Spatially Compact Lyman-alpha Emitting Galaxy at Redshift 5.721
arXiv:astro-ph/0411782 · doi:10.1051/0004-6361:200400126
Abstract
We report the spectroscopic confirmation of a compact \lya emitting galaxy at . A FORS2 spectrum of the source shows a strong asymmetric line with a flux of 5 erg s cm, making it one of the brightest \lya emitting galaxies at this redshift, and a line-of-sight velocity dispersion of 400 km s. We also have a tentative detection of a second, narrower component that is redshifted by 400 km s with respect to the main peak. A FORS2 image shows that the source is compact, with a FWHM of 0\farcs5, which corresponds to 3.2 kpc at this redshift. This source is a brighter example of \object{J1236.8+6215} \citep{Dawson02}, another \lya\ emitting galaxy at .
arXiv commentAccepted by A&A, 4 pages, 4 figures. High resolution figures are available via http://www.mso.anu.edu.au/~westra/publications/
References in corpus (14)
- Absorption-Line Probes of Gas and Dust in Galactic Superwinds
- Probing reionization with Lyman-alpha emission lines
- The Luminosity Function of Lyman Alpha Emitters at Redshift z~5.7
- Spectroscopic Confirmation of Three Redshift 5.7 Lyman-alpha Emitters from the Large Area Lyman Alpha Survey
- Strong Emission Line HII Galaxies in the Sloan Digital Sky Survey. I. Catalog of DR1 Objects with Oxygen Abundances from Te easurements
- The evolution of superbubbles and the detection of Lyman alpha in star-forming galaxies
- The Abundance of Low-luminosity Lyman alpha Emitters at High Redshift
- A Subaru Search for Lyman Emitters at Redshift 5.7
- A Galactic Wind at z = 5.190
- P-Cygni Type Lya from Starburst Galaxies
- One-Line Redshifts and Searches for High-Redshift Lyman-Alpha Emission
- X-ray nondetection of the Lyman-alpha Emitters at z ~ 4.5
- Singly-Peaked P-Cygni type Ly from starburst galaxies
- Constraints to the evolution of Ly-Alpha bright galaxies between z=3 and z=6
Cited by in corpus (20)
- The Subaru/XMM-Newton Deep Survey (SXDS). IV. Evolution of Lya Emitters from z=3.1 to 5.7 in the 1 deg^2 Field: Luminosity Functions and AGN
- The End of the Reionization Epoch Probed by Ly-alpha Emitters at z=6.5 in the Subaru Deep Field
- Completing the Census of Ly-alpha Emitters at the Reionization Epoch
- Lyman alpha emission in high-redshift galaxies
- Constraints on Physical Properties of z~6 Galaxies Using Cosmological Hydrodynamic Simulations
- Systematic Survey of Extended Lyman-alpha Sources over z~3-5
- A z = 3 Lyman Alpha Blob Associated with a Damped Lyman Alpha System Proximate to its Background Quasar
- Serendipitous Discovery of an Overdensity of Lyman-Alpha Emitters at z~4.8 in the Cl1604 Supercluster Field
- HST and Spitzer Observations of the Host Galaxy of GRB 050904: A Metal-Enriched, Dusty Starburst at z=6.295
- A contribution to the selection of emission-line galaxies using narrow-band filters in the optical airglow windows
- A Magellan IMACS Spectroscopic Search for Lyman-Alpha Emitting Galaxies at Redshift 5.7
- Extended Lyman-alpha emission from interacting galaxies at high redshifts
- The DEEP2 Redshift Survey: Lyman Alpha Emitters in the Spectroscopic Database
- On the narrowband detection properties of high-redshift Lyman-alpha emitters
- The properties of the brightest Lyman alpha emitters at z~5.7
- The Wide Field Imager Lyman-Alpha Search (WFILAS) for Galaxies at Redshift ~5.7: II. Survey Design and Sample Analysis
- The Size and Pervasiveness of Ly-UV Spatial Offsets in Star-Forming Galaxies at
- Star Formation Density and Halpha Luminosity Function of an Emission Line Selected Galaxy Sample at z ~ 0.24
- Strong Emission-Line Galaxies at Low Redshift in the Field around the Quasar SDSSp J104433.04-012502.2
- A z ~ 5.7 Lyα Emission Line with an Ultra Broad Red Wing