TY - JOUR
T1 - The hetdex pilot survey. I. Survey design, performance, and catalog of emission-line galaxies
AU - Adams, Joshua J.
AU - Blanc, Guillermo A.
AU - Hill, Gary J.
AU - Gebhardt, Karl
AU - Drory, Niv
AU - Hao, Lei
AU - Bender, Ralf
AU - Byun, Joyce
AU - Ciardullo, Robin
AU - Cornell, Mark E.
AU - Finkelstein, Steven L.
AU - Fry, Alex
AU - Gawiser, Eric
AU - Gronwall, Caryl
AU - Hopp, Ulrich
AU - Jeong, Donghui
AU - Kelz, Andreas
AU - Kelzenberg, Ralf
AU - Komatsu, Eiichiro
AU - MacQueen, Phillip J.
AU - Murphy, Jeremy
AU - Odoms, P. Samuel
AU - Roth, Martin
AU - Schneider, Donald P.
AU - Tufts, Joseph R.
AU - Wilkinson, Christopher P.
PY - 2011/1
Y1 - 2011/1
N2 - We present a catalog of emission-line galaxies selected solely by their emission-line fluxes using a wide-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 □′ with a 3500-5800 Å bandpass under 5 Å full-width-half-maximum (FWHM) spectral resolution. The survey's best sensitivity for unresolved objects under photometric conditions is between 4 and 20 × 10-17 erg s-1 cm-2 depending on the wavelength, and Lya luminosities between 3 × 10 42 and 6 × 1042 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 [Oii]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 Lya 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 □″ which appear to be extended Lyα nebulae. We also find three high-z objects with rest-frame Lya EW above the level believed to be achievable with normal star formation, EW0 > 240 Å. Future papers will investigate the physical properties of this sample.
AB - We present a catalog of emission-line galaxies selected solely by their emission-line fluxes using a wide-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 □′ with a 3500-5800 Å bandpass under 5 Å full-width-half-maximum (FWHM) spectral resolution. The survey's best sensitivity for unresolved objects under photometric conditions is between 4 and 20 × 10-17 erg s-1 cm-2 depending on the wavelength, and Lya luminosities between 3 × 10 42 and 6 × 1042 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 [Oii]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 Lya 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 □″ which appear to be extended Lyα nebulae. We also find three high-z objects with rest-frame Lya EW above the level believed to be achievable with normal star formation, EW0 > 240 Å. Future papers will investigate the physical properties of this sample.
UR - http://www.scopus.com/inward/record.url?scp=78650996540&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=78650996540&partnerID=8YFLogxK
U2 - 10.1088/0067-0049/192/1/5
DO - 10.1088/0067-0049/192/1/5
M3 - Review article
AN - SCOPUS:78650996540
SN - 0067-0049
VL - 192
JO - Astrophysical Journal, Supplement Series
JF - Astrophysical Journal, Supplement Series
IS - 1
ER -