Multi-wavelength landscape of the young galaxy cluster RXJ1257.2+4738 at z=0.866. II. Morphological properties
arXiv:1604.08850 · doi:10.1051/0004-6361/201526744
Abstract
The study of the evolution of the morphological distribution of galaxies in different environments can provide important information about the effects of the environment and the physical mechanisms responsible for the morphological transformations. As part of a complete analysis of the young cluster RXJ1257+4738 at z0.9, we studied in this work the morphological properties of its galaxies. We used non-parametric methods of morphological classification, as implemented in the galSVM code. The classification with the applied method was possible even using ground-based observations: r'-band imaging from OSIRIS/GTC. We defined very conservative probability limits, taking into account the probability errors, in order to obtain a trustworthy classification. In this way we were able to classify about the 30% of all cluster members, and to separate between LT and ET galaxies. Additionally, when analysing the colour-magnitude diagram, we observed a significant population of blue ET galaxies between the classified ones. We discussed possible explanations for the finding of this population. Moreover, we studied different physical properties of LT, ET, and blue ET galaxies. They turn out to be comparable, with the exception of the stellar mass that shows that the red ET population is more massive. We also analysed the morphology-density and morphology-radius relations, observing that, only when considering the morphological separation between ET and LT galaxies, a mild classical behaviour is obtained. RXJ1257+4738 is a young galaxy cluster, showing a clumpy structure and being still in the process of formation, which could explain the lack of some of the standard morphological relations. This makes this cluster a very attractive case for obtaining the higher resolution data and for studying in more details the morphological properties of the entire cluster and relation with the environment.
arXiv comment19 pages, 20 figures. Accepted for publication in A&A
References in corpus (51)
- Astropy: A Community Python Package for Astronomy
- Stellar population synthesis at the resolution of 2003
- Star Formation in Galaxies Along the Hubble Sequence
- Accurate photometric redshifts for the CFHT Legacy Survey calibrated using the VIMOS VLT Deep Survey
- The Sloan Digital Sky Survey Photometric Camera
- The reversal of the star formation-density relation in the distant universe
- Nuclear Activity in Nearby Galaxies
- GOODS-Herschel: an infrared main sequence for star-forming galaxies
- Mid-Infrared Selection of Active Galaxies
- A New Non-Parametric Approach to Galaxy Morphological Classification
- A comprehensive classification of galaxies in the SDSS: How to tell true from fake AGN?
- A Direct Measurement of Major Galaxy Mergers at z < 3
- The Asymmetry of Galaxies: Physical Morphology for Nearby and High Redshift Galaxies
- A Catalog of Detailed Visual Morphological Classifications for 14034 Galaxies in the Sloan Digital Sky Survey
- Subaru Deep Survey V. A Census of Lyman Break Galaxies at z=4 and 5 in the Subaru Deep Fields: Photometric Properties
- A New Approach to Galaxy Morphology: I. Analysis of the Sloan Digital Sky Survey Early Data Release
- The Morphology - Density Relation in z ~ 1 Clusters
- Structural and Photometric Classification of Galaxies - I. Calibration Based on a Nearby Galaxy Sample
- HST Photometry and Keck Spectroscopy of the Rich Cluster MS1054-03: Morphologies, Butcher-Oemler Effect and the Color-Magnitude Relation at z=0.83
- Reversal of Fortune: Confirmation of an Increasing Star Formation-Density Relation in a Cluster at z=1.62
- The STAGES view of red spirals and dusty red galaxies: Mass-dependent quenching of star-formation in cluster infall
- Revisiting the Hubble sequence in the SDSS DR7 spectroscopic sample: a publicly available bayesian automated classification
- The Build-up of the Colour-Magnitude Relation as a Function of Environment
- Galaxy Zoo: A sample of blue early-type galaxies at low redshift
- The Cluster and Field Galaxy AGN Fraction at z = 1 to 1.5: Evidence for a Reversal of the Local Anticorrelation Between Environment and AGN Fraction
- The Morphological Content of Ten EDisCS Clusters at 0.5 < z < 0.8
- A robust morphological classification of high-redshift galaxies using support vector machines on seeing limited images. I Method description
- Clusters at Half Hubble Time: Galaxy Structure and Colors in RXJ0152.7-1357 and MS1054-03
- Spectroscopic Confirmation of Multiple Red Galaxy-Galaxy Mergers in MS1054-03 (z=0.83)
- A Panoramic Mid-infrared Survey of Two Distant Clusters
- LoCuSS: The mid-infrared Butcher-Oemler effect
- New diagnostic methods for emission-line galaxies in deep surveys
- Mass-Selection and the Evolution of the Morphology-Density Relation from z=0.8 to z=0
- The Origin of [OII] in Post-Starburst and Red-Sequence Galaxies in High-Redshift Clusters
- Faint InfraRed Extragalactic Survey: Data and Source Catalogue of the MS1054-03 field
- Morphological Fractions of Galaxies in WINGS Clusters: revisiting the Morphology-Density Paradigm
- From blue star-forming to red passive: galaxies in transition in different environments
- AGN-Host Galaxy Connection: Morphology and Colours of X-ray Selected AGN at z < 2
- Red Star Forming Galaxies and Their Environment at z=0.4 Revealed by Panoramic H-alpha Imaging
- Evolution of blue E/S0 galaxies from z~1: merger remnants or disk rebuilding galaxies?
- The Evolution of Dusty Star formation in Galaxy Clusters to z = 1: Spitzer IR Observations of the First Red-Sequence Cluster Survey
- Reversal or no reversal: the evolution of the star formation rate-density relation up to z~1.6
- The ALHAMBRA survey: reliable morphological catalogue of 22,051 early- and late-type galaxies
- The role of environment in the morphological transformation of galaxies in 9 intermediate redshift clusters
- The impact from survey depth and resolution on the morphological classification of galaxies
- Morphology with Light Profile Fitting of Confirmed Cluster Galaxies at z=0.84
- Multi-wavelength landscape of the young galaxy cluster RXJ1257.2+4738 at z=0.866: I. The infrared view
- Spatial and Kinematic Distributions of Transition Populations in Intermediate Redshift Galaxy Clusters
- On the Reversal of SFR-Density Relation at z=1: Insights from Simulations
- GLACE survey: OSIRIS/GTC Tuneable Filter H imaging of the rich galaxy cluster ZwCl 0024.0+1652 at z = 0.395. Part I -- Survey presentation, TF data reduction techniques and catalogue
- Cluster and cluster galaxy evolution history from IR to X-ray observations of the young cluster RX J1257.2+4738 at z=0.866
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- A morphological study of galaxies in ZwCl0024+1652, a galaxy cluster at redshift z 0.4
- GLACE survey: galaxy activity in ZwCl0024+1652 cluster from strong optical emission lines
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