The Cosmic Evolution Survey (COSMOS): a large-scale structure at z=0.73 and the relation of galaxy morphologies to local environment
arXiv:astro-ph/0701482 · doi:10.1086/516588
Abstract
We have identified a large-scale structure at z~0.73 in the COSMOS field, coherently described by the distribution of galaxy photometric redshifts, an ACS weak-lensing convergence map and the distribution of extended X-ray sources in a mosaic of XMM observations. The main peak seen in these maps corresponds to a rich cluster with Tx= 3.51+0.60/-0.46 keV and Lx=(1.56+/-0.04) x 10^{44} erg/s ([0.1-2.4] keV band). We estimate an X-ray mass within corresponding to M500~1.6 x 10^{14} Msun and a total lensing mass (extrapolated by fitting a NFW profile) M(NFW)=(6+/-3) x 10^15 Msun. We use an automated morphological classification of all galaxies brighter than I_AB=24 over the structure area to measure the fraction of early-type objects as a function of local projected density Sigma_10, based on photometric redshifts derived from ground-based deep multi-band photometry. We recover a robust morphology-density relation at this redshift, indicating, for comparable local densities, a smaller fraction of early-type galaxies than today. Interestingly, this difference is less strong at the highest densities and becomes more severe in intermediate environments. We also find, however, local "inversions'' of the observed global relation, possibly driven by the large-scale environment. In particular, we find direct correspondence of a large concentration of disk galaxies to (the colder side of) a possible shock region detected in the X-ray temperature map and surface brightness distribution of the dominant cluster. We interpret this as potential evidence of shock-induced star formation in existing galaxy disks, during the ongoing merger between two sub-clusters.
15 pages (emulateapj style), 16 figs (low res.); to appear in the ApJ Supplement COSMOS Special Issue. Low-resolution figures; full resolution version available at: http://www.astro.caltech.edu/~cosmos/publications/files/guzzo_0701482.pdf
References in corpus (12)
- The Cosmic Evolution Survey (COSMOS) -- Overview
- Weak Gravitational Lensing with COSMOS: Galaxy Selection and Shape Measurements
- The Shear TEsting Programme 2: Factors affecting high precision weak lensing analyses
- The XMM-Newton wide-field survey in the COSMOS field: VI. Statistical properties of clusters of galaxies
- The high redshift galaxy population in hierarchical galaxy formation models
- COSMOS: 3D weak lensing and the growth of structure
- Large Structures and Galaxy Evolution in COSMOS at z < 1.1
- The XMM-Newton wide-field survey in the COSMOS field II: X-ray data and the logN-logS
- Witnessing galaxy preprocessing in the local Universe: the case of a star-bursting group falling into Abell 1367
- Photometric Redshifts of Galaxies in COSMOS
- The Stability of the Point Spread Function of the Advanced Camera for Surveys on the Hubble Space Telescope and Implications for Weak Gravitational Lensing
- The effects of environment on morphological evolution between 0<z<1.2 in the COSMOS Survey
Cited by in corpus (24)
- The Cosmic Evolution Survey (COSMOS): Subaru Observations of the HST COSMOS Field
- The XMM-Newton wide-field survey in the COSMOS field: I. Survey description
- Stellar and total baryon mass fractions in groups and clusters since redshift 1
- The XMM-Newton wide-field survey in the COSMOS field: VI. Statistical properties of clusters of galaxies
- The STAGES view of red spirals and dusty red galaxies: Mass-dependent quenching of star-formation in cluster infall
- Large Structures and Galaxy Evolution in COSMOS at z < 1.1
- Photometric Redshifts of Galaxies in COSMOS
- A new method to separate star forming from AGN galaxies at intermediate redshift: The submillijansky radio population in the VLA-COSMOS survey
- The effects of environment on morphological evolution between 0<z<1.2 in the COSMOS Survey
- Minor Mergers or Progenitor Bias? The Stellar Ages of Small and Large Quenched Early-Type Galaxies
- STAGES: the Space Telescope A901/2 Galaxy Evolution Survey
- The Complex Structure of the Cl 1604 Supercluster at z~0.9
- AzTEC Millimetre Survey of the COSMOS Field - II. Source Count Overdensity and Correlations with Large-Scale Structure
- (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies - I. Multiwavelength identifications and redshift distribution
- Mass, Light and Colour of the Cosmic Web in the Supercluster SCL2243-0935 (z=0.447)
- A Comparison of Weak Lensing Measurements From Ground- and Space-Based Facilities
- FIR-luminous [CII] emitters in the ALMA-SCUBA-2 COSMOS survey (AS2COSMOS): The nature of submillimeter galaxies in a 10 comoving Mpc-scale structure at z~4.6
- Environmental Effect on the Interstellar Medium in Galaxies across the Cosmic Web at z=0.73
- Towards precise galaxy evolution: a comparison between spectral indices of galaxies in the IllustrisTNG simulation and the LEGA-C survey
- The COSMOS-Web Lens Survey (COWLS) I: Discovery of >100 high redshift strong lenses in contiguous JWST imaging
- Subaru Hyper Suprime-Cam revisits the large-scale environmental dependence on galaxy morphology over 360 deg at z=0.3-0.6
- Large-Scale Fluctuations in the Number Density of Galaxies in Independent Surveys of Deep Fields
- Mapping dark matter and finding filaments: calibration of lensing analysis techniques on simulated data
- The COSMOS Wall at z0.73: star-forming galaxies and their evolution in different environments