Exploring the Diversity of Groups at 0.1<z<0.8 with X-ray and Optically Selected Samples
arXiv:1208.0344 · doi:10.1088/0004-637X/756/2/139
Abstract
We present the global group properties of two samples of galaxy groups containing 39 high quality X-ray selected systems and 38 optically (spectroscopically) selected systems in coincident spatial regions at 0.12<z<0.79. Only nine optical systems are associable with X-ray systems. We discuss the confusion inherent in the matching of both galaxies to extended X-ray emission and of X-ray emission to already identified optical systems. Extensive spectroscopy has been obtained and the resultant redshift catalog and group membership are provided here. X-ray, dynamical, and total stellar masses of the groups are also derived and presented. We explore the effects of applying three different kinds of radial cut to our systems: a constant cut of 1 Mpc and two r200 cuts, one based on the velocity dispersion of the system and the other on the X-ray emission. We find that an X-ray based r200 results in less scatter in scaling relations and less dynamical complexity as evidenced by results of the Anderson-Darling and Dressler-Schectman tests, indicating that this radius tends to isolate the virialized part of the system. The constant and velocity dispersion based cuts can overestimate membership and can work to inflate velocity dispersion and dynamical and stellar mass. We find Lx-sigma and Mstellar-Lx scaling relations for X-ray and optically selected systems are not dissimilar. The mean fraction of mass found in stars for our systems is approximately 0.014 with a logarithmic standard deviation of 0.398 dex. We also define and investigate a sample of groups which are X-ray underluminous given the total group stellar mass. For these systems the fraction of stellar mass contributed by the most massive galaxy is typically lower than that found for the total population of groups implying that there may be less IGM contributed from the most massive member in these systems. (Abridged)
arXiv commentAccepted for publication in the Astrophysical Journal (ApJ). 27 pages, 14 figures, 12 tables
References in corpus (62)
- Stellar population synthesis at the resolution of 2003
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
- A Simple Model for the Absorption of Starlight by Dust in Galaxies
- UV Star Formation Rates in the Local Universe
- Some Aspects of Measurement Error in Linear Regression of Astronomical Data
- The SAURON project - IV. The mass-to-light ratio, the virial mass estimator and the fundamental plane of elliptical and lenticular galaxies
- The Galactic disk mass function: reconciliation of the HST and nearby determinations
- Optimal Techniques in Two-dimensional Spectroscopy: Background Subtraction for the 21st Century
- Galaxy cluster X-ray luminosity scaling relations from a representative local sample (REXCESS)
- The All-wavelength Extended Groth Strip International Survey (AEGIS) Data Sets
- The Average Mass-to-Light Profile of Galaxy Clusters
- Science Objectives and Early Results of the DEEP2 Redshift Survey
- The Properties of Poor Groups of Galaxies: I. Spectroscopic Survey and Results
- Galaxy groups in the 2dFGRS: the group-finding algorithm and the 2PIGG catalogue
- A Census of Baryons in Galaxy Clusters and Groups
- Optical Mass Estimates of Galaxy Clusters
- The GEMS project: X-ray analysis and statistical properties of the group sample
- Galaxy Groups in the SDSS DR4: III. the luminosity and stellar mass functions
- Stellar and total baryon mass fractions in groups and clusters since redshift 1
- Properties of spherical galaxies and clusters with an NFW density profile
- The XMM-Newton wide-field survey in the COSMOS field: VI. Statistical properties of clusters of galaxies
- A Weak Lensing Study of X-ray Groups in the COSMOS survey: Form and Evolution of the Mass-Luminosity Relation
- Constraints on star-formation driven galaxy winds from the mass-metallicity relation at z=0
- The DEEP2 Galaxy Redshift Survey: Evolution of the Color-Density Relation at 0.4 < z < 1.35
- The Lx-T, Lx-sigma and sigma-T relations for groups and clusters of galaxies
- An X-ray Atlas of Groups of Galaxies
- The Properties of Poor Groups of Galaxies: III. The Galaxy Luminosity Function
- Morphological Composition of z~0.4 groups: The site of S0 formation
- The Dawn of the Red: Star formation histories of group galaxies over the past 5 billion years
- LoCuSS: the connection between brightest cluster galaxy activity, gas cooling and dynamical disturbance of X-ray cluster cores
- The DEEP2 galaxy redshift survey: the evolution of the blue fraction in groups and the field
- The stellar mass fraction and baryon content of galaxy clusters and groups
- Microslit Nod-shuffle Spectroscopy - a technique for achieving very high densities of spectra
- HIFLUGCS: Galaxy cluster scaling relations between X-ray luminosity, gas mass, cluster radius, and velocity dispersion
- Evolution of the Internal Dynamics of Galaxy Clusters
- The integrated stellar content of dark matter halos
- Measuring the escape velocity and mass profiles of galaxy clusters beyond their virial radius
- Planck early results: Cluster Sunyaev-Zeldovich optical scaling relations
- The CNOC2 Field Galaxy Redshift Survey I: The Survey and the Catalog for the Patch CNOC 0223+00
- The L_X--M relation of Clusters of Galaxies
- Galaxy Groups at Intermediate Redshift
- Where are the stars?
- Direct observational evidence for a large transient galaxy population in groups at 0.85<z<1
- Galaxy Groups at 0.3 <= z <= 0.55. I. Group Properties
- Statistical Tools for Classifying Galaxy Group Dynamics
- The zCOSMOS Redshift Survey: How group environment alters global downsizing trends
- The LX-sigma Relation for Galaxies and Clusters of Galaxies
- RASS-SDSS Galaxy Cluster Survey. V. The X-ray-Underluminous Abell Clusters
- The roadmap for unification in galaxy group selection:. I. A search for extended X-ray emission in the CNOC2 survey
- The 10k zCOSMOS: morphological transformation of galaxies in the group environment since z~1
- The colour of galaxies in distant groups
- Galaxy Groups at 0.3 <= z <= 0.55. II. Evolution to z ~ 0
- Substructure in the Most Massive GEEC Groups: Field-like Populations in Dynamically Active Groups
- The Evolution of Galaxies in X-ray Luminous Groups
- Do X-ray dark or underluminous galaxy clusters exist?
- An analytic investigation of the scatter in the integrated X-ray properties of galaxy groups and clusters
- Unveiling the Important Role of Groups in the Evolution of Massive Galaxies: Insights from an Infrared Passive Sequence at Intermediate Redshift
- The stellar mass content of distant galaxy groups
- K-band Properties of Well-Sampled Groups of Galaxies
- Evolution in the Disks and Bulges of Group Galaxies since z=0.4
- The CNOC2 Field Galaxy Redshift Survey
- RXJ1648.7+6109: Witnessing the Formation of a Massive Group/Poor Cluster and its Brightest Galaxy
Cited by in corpus (34)
- A luminous X-ray outburst from an intermediate-mass black hole in an off-centre star cluster
- Scaling Properties of Galaxy Groups
- The Complete Local Volume Groups Sample - I. Sample Selection and X-ray Properties of the High-Richness Subsample
- Chandra centres for COSMOS X-ray galaxy groups: Differences in stellar properties between central dominant and offset brightest group galaxies
- LoTSS jellyfish galaxies: II. Ram pressure stripping in groups versus clusters
- Efficient satellite quenching at z~1 from the GEEC2 spectroscopic survey of galaxy groups
- The GEEC2 spectroscopic survey of Galaxy Groups at
- The baryon budget on the galaxy group/cluster boundary
- Mining the gap: evolution of the magnitude gap in X-ray galaxy groups from the 3 square degree XMM coverage of CFHTLS
- Ultra-deep catalog of X-ray groups in the Extended Chandra Deep Field South
- The Growth and Enrichment of the Intragroup Gas
- J1649+2635: A Grand-Design Spiral with a Large Double-Lobed Radio Source
- X-Ray Groups of Galaxies in the Aegis Deep and Wide Fields
- An X-ray Detected Group of Quiescent Early-type Galaxies at z=1.6 in the Chandra Deep Field South
- Structure and substructure analysis of DAFT/FADA galaxy clusters in the [0.4-0.9] redshift range
- The lack of star formation gradients in galaxy groups up to z~1.6
- Stellar Mass to Halo Mass Scaling Relation for X-ray Selected Low Mass Galaxy Clusters and Groups out to Redshift
- Do group dynamics play a role in the evolution of member galaxies?
- Brightest X-ray clusters of galaxies in the CFHTLS wide fields: Catalog and optical mass estimator
- SARCS strong lensing galaxy groups: I - optical, weak lensing, and scaling laws
- The AGN Population in X-ray Selected Galaxy Groups at
- Some Like It Hot: Linking Diffuse X-ray Luminosity, Baryonic Mass, and Star Formation Rate in Compact Groups of Galaxies
- Kinematic unrest of low mass galaxy groups
- Gemini Spectroscopy of Ultra-Compact Dwarfs in the Fossil Group NGC 1132
- The Galaxy Replacement Technique (GRT): a New Approach to Study Tidal Stripping and Formation of Intracluster Light in a Cosmological Context
- Low X-Ray Luminosity Galaxy Clusters. II. Optical properties and morphological content at 0.18 < z < 0.70
- AXES-2MRS: A new all-sky catalogue of extended X-ray galaxy groups
- Toward the low-scatter selection of X-ray clusters: Galaxy cluster detection with eROSITA through cluster outskirts
- The XMM Cluster Survey: Exploring scaling relations and completeness of the Dark Energy Survey Year 3 redMaPPer cluster catalogue
- X-ray cluster cosmology
- The X-Ray Zurich Environmental Study (X-ZENS). II. X-ray Observations of the Diffuse Intragroup Medium in Galaxy Groups
- ALMA measures molecular gas reservoirs comparable to field galaxies in a low-mass galaxy cluster at z=1.3
- Low X-Ray Luminosity Galaxy Clusters: Main goals, sample selection, photometric and spectroscopic observations
- Hyperluminous Supersoft X-Ray Sources in the Chandra Catalog