Journal
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
Volume 192, Issue 1, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0067-0049/192/1/5
Keywords
cosmology: observations; galaxies: evolution; galaxies: formation; galaxies: high-redshift
Categories
Funding
- Texas Norman Hackerman Advanced Research Program [ARP 003658-0005-2006, 003658-0295-2007]
- National Science Foundation
- University of Texas at Austin's William S. Livingston
- National Aeronautics and Space Administration
- NASA [NAS5-26555]
- NASA Office of Space Science [NNX09AF08G]
- David Bruton Jr. Fellowship
- Donald P. Harrington Fellowship
- Direct For Mathematical & Physical Scien [0928636] Funding Source: National Science Foundation
- Division Of Astronomical Sciences [0926641] Funding Source: National Science Foundation
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We present a catalog of emission-line galaxies selected solely by their emission-line fluxes using awide-field integral field spectrograph. This work is partially motivated as a pilot survey for the upcoming Hobby-Eberly Telescope Dark Energy Experiment. We describe the observations, reductions, detections, redshift classifications, line fluxes, and counterpart information for 397 emission-line galaxies detected over 169 square' with a 3500-5800 angstrom bandpass under 5 angstrom full-width-half-maximum (FWHM) spectral resolution. The survey's best sensitivity for unresolved objects under photometric conditions is between 4 and 20 x 10(-17) erg s(-1) cm(-2) depending on the wavelength, and Ly alpha luminosities between 3 x 10(42) and 6 x 10(42) erg s(-1) are detectable. This survey method complements narrowband and color-selection techniques in the search of high-redshift galaxies with its different selection properties and large volume probed. The four survey fields within the COSMOS, GOODS-N, MUNICS, and XMM-LSS areas are rich with existing, complementary data. We find 105 galaxies via their high-redshift Lya emission at 1.9 < z < 3.8, and the majority of the remainder objects are low-redshift [O II] 3727 emitters at z < 0.56. The classification between low-and high-redshift objects depends on rest-frame equivalent width (EW), as well as other indicators, where available. Based on matches to X-ray catalogs, the active galactic nuclei fraction among the Ly alpha emitters is 6%. We also analyze the survey's completeness and contamination properties through simulations. We find five high-z, highly significant, resolved objects with FWHM sizes >44 square '' which appear to be extended Ly alpha nebulae. We also find three high-z objects with rest-frame Ly alpha EW above the level believed to be achievable with normal star formation, EW0 > 240 angstrom. Future papers will investigate the physical properties of this sample.
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