Directly imaging damped Ly-alpha galaxies at z>2. II: Imaging and spectroscopic observations of 32 quasar fields
arXiv:1404.2599 · doi:10.1093/mnras/stu1512
Abstract
Damped Ly-alpha absorbers (DLAs) are a well-studied class of absorption line systems, and yet the properties of their host galaxies remain largely unknown. To investigate the origin of these systems, we have conducted an imaging survey of 32 quasar fields with intervening DLAs between z~1.9-3.8, leveraging a technique that allows us to image galaxies at any small angular separation from the background quasars. In this paper, we present the properties of the targeted DLA sample, new imaging observations of the quasar fields, and the analysis of new and archival spectra of the background quasars.
arXiv comment76 pages, 48 figures, 28 tables. To appear in MNRAS
References in corpus (48)
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- The chemical composition of the Sun
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Measuring Reddening with SDSS Stellar Spectra and Recalibrating SFD
- Correcting for the Effects of Interstellar Extinction
- Cosmic-Ray Rejection by Laplacian Edge Detection
- The u'g'r'i'z' Standard Star Network
- X-shooter, the new wide band intermediate resolution spectrograph at the ESO Very Large Telescope
- Damped Lyman alpha Systems
- CANDELS Multi-wavelength Catalogs: Source Detection and Photometry in the GOODS-South Field
- The Sloan Digital Sky Survey Quasar Catalog IV. Fifth Data Release
- A Modified Magnitude System that Produces Well-Behaved Magnitudes, Colors, and Errors Even for Low Signal-to-Noise Ratio Measurements
- ESI, a new Keck Observatory echellette spectrograph and imager
- Column density distribution and cosmological mass density of neutral gas: Sloan Digital Sky Survey-III Data Release 9
- On the (Non)Evolution of HI Disks over Cosmic Time
- CANDELS Multiwavelength catalogs: Source Identification and Photometry in the CANDELS UKIDSS Ultra-Deep Survey Field
- Metallicity Evolution of Damped Lyman-alpha Systems out to z~5
- The Age-Metallicity Relation of the Universe in Neutral Gas: The First 100 Damped Lya Systems
- Evolution of the cosmological mass density of neutral gas from Sloan Digital Sky Survey II - Data Release 7
- The Multiwavelength Survey by Yale-Chile (MUSYC): Survey Design and Deep Public UBVRIz' Images and Catalogs of the Extended Hubble Deep Field South
- Velocity-Metallicity Correlation for high-z DLA Galaxies: Evidence for a Mass-Metallicity Relation?
- A Population of Faint Extended Line Emitters and the Host Galaxies of Optically Thick QSO Absorption Systems
- Extended Ly-alpha emission from a damped Ly-alpha absorber at z = 1.93, and the relation between DLAs and Lyman-break galaxies
- The ESO UVES Advanced Data Products Quasar Sample - II. Cosmological Evolution of the Neutral Gas Mass Density
- The ESI/KeckII Damped Lya Abundance Database
- The Rapid Decline in Metallicity of Damped Ly-alpha Systems at z~5
- Mass-metallicity relation from z=5 to the present: Evidence for a transition in the mode of galaxy growth at z=2.6 due to the end of sustained primordial gas infall
- Galaxy Counterparts of metal-rich Damped Lyman-alpha Absorbers - I: The case of the z=2.35 DLA towards Q2222-0946
- The Fundamental Plane of Damped Lyman Alpha Systems
- The Ucsd/Keck Damped Lya Abundance Database: A Decade of High Resolution Spectroscopy
- MASE: A New Data--Reduction Pipeline for the Magellan Echellette Spectrograph
- Discovery of a compact gas-rich DLA galaxy at z = 2.2: evidences for a starburst-driven outflow
- A SINFONI Integral Field Spectroscopy Survey for Galaxy Counterparts to Damped Lyman-alpha Systems - I. New Detections and Limits for Intervening and Associated Absorbers
- Dissecting the properties of optically-thick hydrogen at the peak of cosmic star formation history
- The Nature of Damped Lyman Alpha Systems and Their Hosts in the Standard Cold Dark Matter Universe
- HST Images of a Galaxy Group at z=2.81, and the Sizes of Damped Lyman Alpha Galaxies
- NICMOS imaging search for damped Lya galaxies
- On the sizes of z>2 Damped Lyman-alpha Absorbing Galaxies
- Distribution of Damped Lyman-alpha Absorbers in a Lambda Cold Dark Matter Universe
- The Magellan Uniform Survey of Damped Lyman alpha Systems I: Cosmic Metallicity Evolution
- Bimodality in Damped Lyman alpha Systems
- PMN J1838-3427: A new gravitationally lensed quasar
- Spatially Resolved Emission of a High Redshift DLA Galaxy with the Keck/OSIRIS IFU
- Directly imaging damped Lyman-alpha galaxies at z>2. I: Methodology and First Results
- Survey for Galaxies Associated with z~3 Damped Lyman alpha Systems I: Spectroscopic Calibration of u'BVRI Photometric Selection
- A Shot in the Dark: A Technique for Locating the Stellar Counterparts of Damped Lyman Alpha Absorbers
- Uncovering strong MgII absorbing galaxies: Imaging below the Lyman limit
- Fixing the U-band photometry of Type Ia supernovae
Cited by in corpus (34)
- Four phases of angular-momentum buildup in high-z galaxies: from cosmic-web streams through an extended ring to disc and bulge
- Consensus report on 25 years of searches for damped Ly galaxies in emission: Confirming their metallicity-luminosity relation at
- A halo model for cosmological neutral hydrogen: abundances and clustering
- MUSE searches for galaxies near very metal-poor gas clouds at z~3: new constraints for cold accretion models
- The most metal-poor damped Lyman alpha systems: An insight into dwarf galaxies at high redshift
- Directly imaging damped Ly-alpha galaxies at z>2. III: The star formation rates of neutral gas reservoirs at z~2.7
- Unveiling the Secrets of Metallicity and Massive Star Formation Using DLAs along Gamma-ray Bursts
- Dissecting the Gaseous Halos of z~2 Damped Ly Systems with Close Quasar Pairs
- MUSE Analysis of Gas around Galaxies (MAGG) -- I: Survey design and the environment of a near pristine gas cloud at z~3.5
- Witnessing galaxy assembly in an extended z~3 structure
- Constraining a halo model for cosmological neutral hydrogen
- A study of the circum-galactic medium at z ~ 0.6 using DLA-galaxies
- MUSE Analysis of Gas around Galaxies (MAGG) -- IV: The gaseous environment of 3-4 Lyman-alpha emitting galaxies
- Linking gas and galaxies at high redshift: MUSE surveys the environments of six damped Lyman alpha galaxies at z~3
- The Effect Of AGN Heating On The Low-Redshift Lyα Forest
- ALMA + VLT observations of a Damped Lyman-α absorbing galaxy: Massive, wide CO emission, gas-rich but with very low SFR
- The Mean Metal-line Absorption Spectrum of DLAs in BOSS
- Characterising the Circum-Galactic Medium of Damped Lyman- Absorbing Galaxies
- Modelling the cosmic neutral hydrogen from DLAs and 21 cm observations
- The Star Formation Rate Efficiency of Neutral Atomic-dominated Hydrogen Gas in the Outskirts of Star Forming Galaxies from z~1 to z~3
- Statistical properties of Faraday rotation measure in external galaxies -- I: intervening disc galaxies
- Robust automatic photometry of local galaxies from SDSS Dissecting the color magnitude relation with color profiles
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: The Damped Lyman- systems Catalog
- A search for H emission in high-metallicity damped Lyman- systems at
- Discovery of a Damped Lya Absorber at z = 3.3 along a galaxy sight-line in the SSA22 field
- The gas and stellar mass of low-redshift damped Lyman- absorbers
- HI 21cm emission from the sub-damped Lyman-alpha absorber at z=0.0063 towards PG1216+069
- A Multi-messenger view of Cosmic Dawn: Conquering the Final Frontier
- Exploring Damped Lyman- System Host Galaxies using Gamma-ray Bursts
- The Physical Nature of the Most Metal-Poor Damped Lyman Alpha Systems
- A [CII]-158-micron Survey of DLA galaxies at z~4: Observations of Dense and Metal-Enriched Neutral Gas within the Circumgalactic Medium of Star-Forming Galaxies
- Discovery of a damped Ly galaxy at z 3 towards the quasar SDSS J011852+040644
- Inferring the Distances of Fast Radio Bursts Through Associated 21-cm Absorption
- Star-Formation in Neutral Hydrogen Gas Reservoirs at Cosmic Noon