Science Objectives and Early Results of the DEEP2 Redshift Survey

Abstract

The DEIMOS spectrograph has now been installed on the Keck-II telescope and commissioning is nearly complete. The DEEP2 Redshift Survey, which will take approximately 120 nights at the Keck Observatory over a three year period and has been designed to utilize the power of DEIMOS, began in the summer of 2002. The multiplexing power and high efficiency of DEIMOS enables us to target 1000 faint galaxies per clear night. Our goal is to gather high-quality spectra of \~60,000 galaxies with z>0.75 in order to study the properties and large scale clustering of galaxies at z ~ 1. The survey will be executed at high spectral resolution, $R=\lambda /\Delta \lambda \approx 5000$, allowing us to work between the bright OH sky emission lines and to infer linewidths for many of the target galaxies (for several thousand objects, we will obtain rotation curves as well). The linewidth data will facilitate the execution of the classical redshift-volume cosmological test, which can provide a precision measurement of the equation of state of the Universe. This talk reviews the project, summarizes our science goals and presents some early DEIMOS data.

12 pages, 5 figures, talk presented at SPIE conference, Aug. 2002

Cited by in corpus (424)

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• Calibrating the Star Formation Rate at z=1 from Optical Data
• The hierarchical build-up of the Tully-Fisher relation
• Dwarf Galaxies in the Coma Cluster: I. Velocity Dispersion Measurements
• Multi-Wavelength Study of a Complete IRAC 3.6micron-Selected Galaxy Sample: a Fair Census of Red and Blue Populations at Redshifts 0.4-1
• Implications of the Environments of Radio-detected AGN in a Complex Protostructure at z$\sim$3.3
• The Stellar Population and Star Formation Rates of z~1.5-1.6 [O II] Emitting Galaxies Selected from Narrow-Band Emission-Line Surveys
• DES Science Portal: Computing Photometric Redshifts
• Observational constraints on the physics behind the evolution of AGN since z ~ 1
• Evidence for (and Against) Progenitor Bias in the Size Growth of Compact Red Galaxies
• The impact of the Star Formation Histories on the SFR-M${}_{\ast }$ relation at z$\ge$2
• Exploring Galaxy Formation Models and Cosmologies with Galaxy Clustering
• The X-ray Properties of Moderate-redshift Galaxy Groups Selected by Association with Gravitational Lenses
• The kinematic footprints of five stellar streams in Andromeda's halo
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• The PAU Survey: Measurement of Narrow-band galaxy properties with Approximate Bayesian Computation
• Host Galaxies of z=4 Quasars
• Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model - I. Magnitude counts, redshift distribution, colour bimodality, and galaxy clustering
• Observations of Mg II Absorption Near z ~ 1 Galaxies Selected From The DEEP2 Redshift Survey
• The WIRCam Deep Survey II: Mass Selected Clustering
• The metallicities of luminous, massive field galaxies at intermediate redshifts
• First Systematic Search for Oxygen-Line Blobs at High Redshift: Uncovering AGN Feedback and Star-Formation Quenching
• Photometric Objects around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. I. Methods
• A 16 deg${}^2$ survey of emission-line galaxies at z<1.6 from HSC-SSP PDR2 and CHORUS
• The Space Density Evolution of Wet and Dry Mergers in the Canada-France-Hawaii Telescope Legacy Survey
• Non-Gaussian gravitational clustering field statistics
• A robust lower limit on the amplitude of matter fluctuations in the universe from cluster abundance and weak lensing
• BH Accretion in Low-Mass Galaxies Since z~1
• Quasi-stellar objects in the ALHAMBRA survey. I. Photometric redshift accuracy based on a 23 optical-NIR filter photometry
• X-ray Groups of Galaxies at 0.5<z<1 in zCOSMOS: Increased AGN Activities in High Redshift Groups
• The Hunt for Red Quasars: Luminous Obscured Black Hole Growth Unveiled in the Stripe 82 X-ray Survey
• AEGIS: Chandra Observation of DEEP2 Galaxy Groups and Clusters
• The Role of Galaxy Interaction in Environmental Dependence of the Star Formation Activity at z~1.2
• Groups of Galaxies in AEGIS: The 200 ksec Chandra Extended X-ray Source catalogue
• Protocluster detection in simulations of HSC-SSP and the 10-year LSST forecast, using PCcones
• Evolution of the Fundamental Plane of 0.2<z<1.2 Early-type galaxies in the EGS
• The Origin of [OII] Emission in Recently Quenched AGN Hosts
• PRIMUS: Obscured Star Formation on the Red Sequence
• Maturing Satellite Kinematics into a Competitive Probe of the Galaxy-Halo Connection
• Inferring the photometric and size evolution of galaxies from image simulations
• Eigenmode Analysis of Galaxy Distributions in Redshift Space
• Improved Mock Galaxy Catalogs for the DEEP2 Galaxy Redshift Survey from Subhalo Abundance and Environment Matching
• Dust attenuation in the restframe ultraviolet: constraints from star-forming galaxies at z~1
• Effects of galaxy environment on merger fraction
• Spectral classification of emission-line galaxies from the Sloan Digital Sky Survey. II. A supplementary diagnostic for AGNs using the Dn(4000) index
• Probability Friends-of-Friends (PFOF) Group Finder: Performance Study and Observational Data Applications on Photometric Surveys
• Exploring the High-Mass End of the Stellar Mass Function of Star Forming Galaxies at Cosmic Noon
• The Environment on few Mpc scales of Infrared Luminous Galaxies at Redshifts z~1
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. III. Accurate Measurement of Galaxy Stellar Mass Function with the Aid of Cosmological Redshift Surveys
• The Properties of Radio and Mid-infrared Detected Galaxies and the Effect of Environment on the Co-evolution of AGN and Star Formation at $z\sim 1$
• The DEEP2 Galaxy Redshift Survey: Redshift Identification of Single-Line Emission Galaxies
• The VIMOS VLT Deep Survey: Testing the gravitational instability paradigm at z ~ 1
• The PAU Survey: Measurements of the 4000 Å spectral break with narrow-band photometry
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. IV. High Precision Constraints on the Evolution of Stellar-Halo Mass Relation at Redshift $z<0.7$
• The structure of the merging RCS 231953+00 Supercluster at z ~ 0.9
• Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model. II. The colour-density relation up to z=1.5
• Dissecting the Power Sources of Low-Luminosity Emission-Line Galaxy Nuclei via Comparison of HST-STIS and Ground-Based Spectra
• Next Generation Virgo Cluster Survey. XXI. The weak lensing masses of the CFHTLS and NGVS RedGOLD galaxy clusters and calibration of the optical richness
• The Dark Matter Haloes and Host Galaxies of MgII Absorbers at z~1
• Simulated evolution of the dark matter large-scale structure
• Discovering Large-Scale Structure at $2<z<5$ in the C3VO Survey
• Dynamical analysis of strong-lensing galaxy groups at intermediate redshift
• The Coevolution of Massive Quiescent Galaxies and Their Dark Matter Halos over the Last 6 Billion Years
• Can We Detect the Color-Density Relation with Photometric Redshifts?
• A Fully-Identified Sample of AEGIS20 Microjansky Radio Sources
• Spectroscopy of Luminous Compact Blue Galaxies in Distant Clusters I. Spectroscopic Data
• Mid-infrared Identification of 6 cm Radio Source Counterparts in the Extended Groth Strip
• Bulgeless Galaxies at Intermediate Redshift: Sample Selection, Colour Properties, and the Existence of Powerful AGN
• The WIRCam Ultra Deep Survey (WUDS) I. Survey overview and UV luminosity functions at z~5 and z~6
• Probing nuclear activity versus star formation at z~0.8 using near-infrared multi-object spectroscopy
• HI imaging of dwarf star-forming galaxies: Masses, morphologies and gas deficiencies
• The Tully-Fisher Relation in Cluster Cl0024+1654 at z=0.4
• A spectroscopic measure of the star-formation rate density in dwarf galaxies at z~1
• Shining Light on Merging Galaxies I: The Ongoing Merger of a Quasar with a `Green Valley' Galaxy
• Star Formation In The Cluster Merger DLSCL J0916.2+2953
• Using galaxy pairs as cosmological tracers
• Order statistics of the early-type galaxy luminosity function
• The ESO-Sculptor Survey: Evolution of late-type galaxies at redshifts 0.1-0.5
• The nature of H$\alpha$-selected galaxies along the large-scale structure at z=0.4 revealed by Subaru Hyper Suprime-Cam survey
• An accurate new method of calculating absolute magnitudes and K-corrections applied to the Sloan filter set
• The PAU Survey: Photometric redshift estimation in deep wide fields
• The WiggleZ Dark Energy Survey: Star-formation in UV-luminous galaxies from their luminosity functions
• The WHIQII Survey: Metallicities and Spectroscopic Properties of Luminous Compact Blue Galaxies
• Star formation rates and chemical abundances of emission line galaxies in intermediate-redshift clusters
• Measuring Stellar Masses of Emission Line Galaxies at 1.2<z<1.9
• Optimizing high redshift galaxy surveys for environmental information
• Constraints on the evolutionary mechanisms of massive galaxies since $z\sim 1$ from their velocity dispersions
• AEGIS: Galaxy Spectral Energy Distributions from the X-Ray to Radio
• COMBO-17 measurements of the effect of environment on the type-dependent galaxy luminosity function
• Predicting spectral features in galaxy spectra from broad-band photometry
• The Halo Masses of Galaxies to $z\sim 3$: A Hybrid Observational and Theoretical Approach
• The H$\alpha$ and [O III] $\lambda 5007$ Luminosity Functions of $1.2<z<1.9$ Emission-Line Galaxies from HST Grism Spectroscopy
• The Dwarf Galaxy Population at $z\sim 0.7$: A Catalog of Emission Lines and Redshifts from Deep Keck Observations
• X-ray Surface Brightness Profiles of Optically Selected Active Galactic Nuclei: Comparison with X-ray AGN
• SED-inferred properties and morphology of Lyman-break galaxies at $z\sim 1$ in the CDF-S
• Development of SED Camera for Quasars in Early Universe (SQUEAN)
• Dark Energy Survey Deep Field photometric redshift performance and training incompleteness assessment
• Photometric IGM tomography with Subaru/HSC: the large-scale structure of Ly$\alpha$ emitters and IGM transmission in the COSMOS field at $z\sim 5$
• The nebular properties of star-forming galaxies at intermediate redshift from the Large Early Galaxy Astrophysics Census
• Disentangling the physical origin of emission line ratio offsets at high redshift with spatially resolved spectroscopy
• Environmental impact on star-forming galaxies in a $z\sim 0.9$ cluster during course of galaxy accretion
• Environmental Effects in the Evolution of Galactic Bulges
• An X-ray/optical study of the geometry and dynamics of MACS J0140.0-0555, a massive post-collision cluster merger
• The Redshift-Space Two Point Correlation Function of ELAIS-S1 Galaxies
• FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking
• On the Origin of the Strong Optical Variability of Emission-line Galaxies
• Kinematic Lensing Inference II: Cluster Lensing with $\mathcal{O}$(1) Galaxies
• Selecting Clusters and Protoclusters via Stellar Mass Density: II. Application to HSC-SSP Observations
• Oxford SWIFT IFS and multi-wavelength observations of the Eagle galaxy at z=0.77
• Comparison of the spatial and the angular clustering of X-ray AGN
• Observing the high redshift universe using the VIMOS-IFU
• Photometric Selection of a Massive Galaxy Catalog with $z\ge 0.55$
• The History of Galaxy Formation in Groups: An Observational Perspective