A Study of Nine High-Redshift Clusters of Galaxies: II. Photometry, Spectra, and Ages of Clusters 0023+0423 and 1604+4304
arXiv:astro-ph/9805155 · doi:10.1086/300463
Abstract
We present an extensive photometric and spectroscopic study of two high-redshift clusters of galaxies based on data obtained from the Keck 10m telescopes and the Hubble Space Telescope. The clusters CL0023+0423 (z=0.84) and CL1604+4304 (z=0.90) are part of a multi-wavelength program to study nine candidate clusters at z > 0.6 (Oke, Postman & Lubin 1998). Based on these observations, we study in detail both the field and cluster populations. From the confirmed cluster members, we find that CL0023+0423 actually consists of two components separated by ~2900 km/s. A kinematic analysis indicates that the two components are a poor cluster with ~3 x 10^{14} solar masses and a less massive group with 10^{13} solar masses. CL1604+4304 is a centrally concentrated, rich cluster at z = 0.8967 with a velocity dispersion of 1226 km/s and a mass of ~3 x 10^{15} solar masses. Approximately 57% and 50% of the galaxies show high levels of star formation in CL0023+0423 and CL1604+4304, respectively. These numbers are significantly larger than those found in intermediate redshift clusters. We also observe many old, red galaxies. Found mainly in CL1604+4304, they have spectra consistent with passive stellar evolution, typical of the early-type galaxies in low and intermediate-redshift clusters. We have calculated their ages by comparing their spectral energy distributions to standard Bruzual & Charlot evolutionary models. We find that their colors are consistent with models having an exponentially decreasing star formation rate with a time constant of 0.6 Gyr. We observe a significant luminosity brightening in our brightest cluster galaxies. Compared to BCGs at z < 0.1, we find a luminosity increase of ~1 mag in the rest B-band and ~0.8 mag in the rest V-band.
arXiv comment65 pages, 21 figures. (Two are large plate images available from the lead author). Accepted for publication in the Astronomical Journal
References in corpus (26)
- The Star Formation History of Field Galaxies
- Evolution since z = 0.5 of the Morphology-Density relation for Clusters of Galaxies
- The Evolution of Early-Type Galaxies in Distant Clusters
- The Properties of Poor Groups of Galaxies: I. Spectroscopic Survey and Results
- The CANADA-FRANCE REDSHIFT SURVEY VI: Evolution of the galaxy luminosity function to z ~ 1
- Galaxy Cluster Virial Masses and Omega
- The Homogeneity of Spheroidal Populations in Distant Clusters
- K and evolutionary corrections from UV to IR
- The Luminosity-Temperature Relation at z=0.4 for Clusters of galaxies
- Star Formation in Cluster Galaxies at 0.2<z<0.55
- Galaxy Evolution in Abell 2390
- CFRS XIV: Spectral Properties Of Field Galaxies Up To z = 1
- Deep optical galaxy counts with the Keck Telescope
- Redshift clustering in the Hubble Deep Field
- A Catalog of Morphological Types in 10 Distant Rich Clusters of Galaxies
- EVOLUTION OF IR-SELECTED GALAXIES IN Z~0.4 CLUSTERS
- A wide-field K-band survey - I. Galaxy counts in B, V, I and K
- The Norris Survey of the Corona Borealis Supercluster: III. Structure and Mass of the Supercluster
- Detection of Massive Forming Galaxies at Redshifts Greater than One
- A Study of Nine High-Redshift Clusters of Galaxies : III. HST Morphology of Clusters 0023+0423 and 1604+4304
- A Study of Nine High-Redshift Clusters of Galaxies: I. The Survey
- Redshift z ~ 1 Field Galaxies Observed with the Keck Telescope and the HST
- A Dynamical Study of Optically Selected Distant Clusters
- The Palomar Distant Cluster Survey : III. The Colors of the Cluster Galaxies
- A Group-Group Merger at a Redshift of z = 0.84?
- Strong Redshift Clustering of Distant Galaxies
Cited by in corpus (84)
- A New Method For Galaxy Cluster Detection I: The Algorithm
- The Morphology - Density Relation in z ~ 1 Clusters
- The evolution of the star formation activity in galaxies and its dependence on environment
- A JavaScript Passive Evolution Calculator
- HST Photometry and Keck Spectroscopy of the Rich Cluster MS1054-03: Morphologies, Butcher-Oemler Effect and the Color-Magnitude Relation at z=0.83
- A comparison of the galaxy populations in the Coma and distant clusters: the evolution of k+a galaxies and the role of the intracluster medium
- The Build-up of the Colour-Magnitude Relation as a Function of Environment
- Hubble Space Telescope weak lensing study of the z=0.83 cluster MS 1054-03
- The zCOSMOS Redshift Survey: the role of environment and stellar mass in shaping the rise of the morphology-density relation from z~1
- Halpha-Derived Star-Formation Rates For Three z ~ 0.75 EDisCS Galaxy Clusters
- Evolution of the Internal Dynamics of Galaxy Clusters
- ROSAT-SDSS Galaxy Clusters Survey. I. The Catalog and the correlation of X-ray and optical properties
- A Panoramic Halpha Imaging Survey of the z=0.4 cluster Cl0024.0+1652 with Subaru
- The Angular Clustering of Distant Galaxy Clusters
- B2045+265: A New Four-Image Gravitational Lens from CLASS
- Spectroscopy of clusters in the ESO Distant Cluster Survey (EDisCS)
- A Study of Nine High-Redshift Clusters of Galaxies: IV. Photometry and Sp ectra of Clusters 1324+3011 and 1604+4321
- The Observations of Redshift Evolution in Large Scale Environments (ORELSE) Survey : I. The Survey Design and First Results on Cl 0023+0423 at z = 0.84 and RX J1821.6+6827 at z = 0.82
- IR observations of MS 1054-03: Star Formation and its Evolution in Rich Galaxy Clusters
- Spectroscopy of clusters in the ESO distant cluster survey (EDisCS).II. Redshifts, velocity dispersions, and substructure for clusters in the last 15 fields
- Velocity Dispersion of 335 Galaxy Clusters Selected from the Sloan Digital Sky Survey: Statistical Evidence for Dynamical Interaction, and Against Ram-Pressure Stripping
- A VLT spectroscopic survey of RX J0152.7-1357, a forming cluster of galaxies at z=0.837
- The Tolman Surface Brightness Test for the Reality of the Expansion. IV. A Measurement of the Tolman Signal and the Luminosity Evolution of Early-Type Galaxies
- Distant Cluster Hunting II: A comparison of X-ray and optical cluster detection techniques and catalogs from the ROX Survey
- A Study of Nine High-Redshift Clusters of Galaxies : III. HST Morphology of Clusters 0023+0423 and 1604+4304
- Spectroscopic Confirmation of the Cl 1604 Supercluster at z~0.9
- The Complex Structure of the Cl 1604 Supercluster at z~0.9
- RXJ1716.6+6708: a young cluster at z=0.81
- An HST Search for Lyman Continuum Emission From Galaxies at z=1.1--1.4
- Dynamical state and star formation properties of the merging galaxy cluster Abell 3921
- A Study of Nine High-Redshift Clusters of Galaxies: I. The Survey
- A Definitive Optical Detection of a Supercluster at z = 0.91
- Evidence for Cluster Evolution from an Improved Measurement of the Velocity Dispersion and Morphological Fraction of Cluster 1324+3011 at z = 0.76
- The Gravitational Lens -- Galaxy Group Connection: I. Discovery of a Group Coincident with CLASS B0712+472
- The First Detailed X-ray Observations of High-Redshift, Optically-Selected Clusters: XMM-Newton Results for Cl 1324+3011 at z = 0.76 and Cl 1604+4304 at z = 0.90
- Distant Cluster Hunting I: A Comparison Between the Optical and X-ray Luminosity Functions from an Optical/X-ray Survey
- The XMM-LSS Survey. First high redshift galaxy clusters: relaxed and collapsing systems
- Internal dynamics of the radio--halo cluster A2219: a multi-wavelength analysis
- The Evolution of Galaxies in X-ray Luminous Groups
- The Red Sequence Luminosity Function in Massive Intermediate Redshift Galaxy Clusters
- Detection of Dark Matter Concentrations in the Field of Cl 1604+4304 from Weak Lensing Analysis
- HST/ACS weak lensing analysis of the galaxy cluster RDCS 1252.9-2927 at z=1.24
- The Luminosity Functions of the Galaxy Cluster MS1054-0321 at z=0.83 based on ACS Photometry
- Caltech Faint Galaxy Redshift Survey VIII: Analysis for the Field J0053+1234
- H-Derived Star-Formation Rates for the z=0.84 Galaxy Cluster CLJ0023+0423B
- The Tolman Surface Brightness Test for the Reality of the Expansion. I. Calibration of the Necessary Local Parameters
- Internal dynamics of the radio halo cluster Abell 773: a multiwavelength analysis
- The Hubble Space Telescope Cluster Supernova Survey: III. Correlated Properties of Type Ia Supernovae and Their Hosts at 0.9 < z < 1.46
- Chandra Observations of the Cl1604 Supercluster at z=0.9: Evidence for an Overdensity of Active Galactic Nuclei
- A Probabilistic Quantification of Galaxy Cluster Membership
- Galaxy Population in a Cluster of Galaxies around the Radio Galaxy 3C 324 at z=1.2
- Do star formation rates of galaxy clusters depend on mass?: blue/late-type fractions, total star formation rates of 115 galaxy clusters as a function of cluster virial mass
- Extremely Red Objects in the Field of QSO 1213-0017: A Galaxy Concentration at z=1.31
- RASS-SDSS Galaxy Cluster Survey. VI. The dependence of the cluster SFR on the cluster global properties
- Obscured Starburst Activity in High Redshift Clusters and Groups
- Ram-Pressure Stripping of Galaxies in High-Redshift Clusters and Influence of ICM Heating
- A Group-Group Merger at a Redshift of z = 0.84?
- Cluster of galaxies around seven radio-loud QSOs at 1<z<1.6: K-band images
- The Properties of Radio Galaxies and the Effect of Environment in Large Scale Structures at
- Properties of Galaxies Hosting X-ray Selected Active Galactic Nuclei in the Cl1604 Supercluster at z=0.9
- A Rich Cluster of Galaxies Near the Quasar B2 1335+28 at z=1.1: Color Distribution and Star-Formation Properties
- Weak Lensing Detection of Cl 1604+4304 at z = 0.90
- Pushing the Boundaries of the Cl 1604 Supercluster at z~0.9
- Are Passive Spiral Galaxies Truly "Passive" and "Spiral"? : Near-Infrared Perspective
- The Formation Epoch of Early-Type Galaxies in the z ~ 0.9 CL1604 Supercluster
- Velocity segregation effects in galaxy clusters at 0.4<~z<~1.5
- The Evolution and Environments of X-ray Emitting Active Galactic Nuclei in High-Redshift Large-Scale Structures
- The Evolution of [OII] Emission from Cluster Galaxies
- An excess of sub-millimetre sources towards z~1 clusters
- The X-ray-Optical Relations for Nine Clusters at z = 0.7-1.1
- Imprints of Environment on Cluster and Field Late-type Galaxies at z~1
- Testing Weak Lensing Maps With Redshift Surveys: A Subaru Field
- Spectroscopic confirmation of a cluster of galaxies at z=1 in the field of the gravitational lens MG2016+112
- The structure of the merging RCS 231953+00 Supercluster at z ~ 0.9
- The Tolman Surface Brightness Test for the Reality of the Expansion. III. HST Profile and Surface Brightness Data for Early-Type Galaxies in Three High-Redshift Clusters
- Isophote Shapes of Early-Type Galaxies in Massive Clusters at and 0
- Active Galactic Nuclei in the CNOC2 Field Galaxy Redshift Survey
- The Tolman Surface Brightness Test for the Reality of the Expansion. II. The Effect of the Point-Spread Function and Galaxy Ellipticity on the Derived Photometric Parameters
- The Tolman Surface Brightness Test for the Reality of the Expansion. V. Provenance of the Test and a New Representation of the Data for Three Remote HST Galaxy Clusters
- Color, spectral and morphological transformations of galaxies in clusters
- Cl 1103.7-1245 at z=0.96: the highest redshift galaxy cluster in the EDisCS survey
- No Evidence of Quasar-Mode Feedback in a Four-Way Group Merger at z~0.84
- Emission line galaxies in clusters
- The intermediate-redshift galaxy cluster CL 0048-2942. Stellar populations