The Evolution of Early-Type Galaxies in Distant Clusters I.: Surface Photometry and Structural Parameters for 53 Galaxies in the z=0.33 Cluster CL1358+62
arXiv:astro-ph/9911065 · doi:10.1086/308460
Abstract
Using HST imaging of CL1358+62 (z=0.33) structural parameters are derived for 53 cluster members. We fit integrated r^{1/4}-laws to the integrated S.B. profiles, and fit two-dimensional r^{1/4}-law model galaxies to the images directly. The results from the two methods agree very well, with an rms scatter of 13% in r_e. The half-light radii range from 1 to 20 kpc, with a median of 3 kpc. We compared r_e from the r^{1/4}-law fits to r_{1/2} derived using other profiles. In particular, we fit Sersic r^{1/n}-laws and superpositions of r^{1/4}-law bulges with exponential disks. The r_{1/2} derived from the best-fit Sersic profiles varied with respect to r_e from the r^{1/4}-law fits by 1% in the median, but with a standard deviation of more than 40%. For the bulge-plus-disk fits, the derived r_{1/2} were offset from r_e of the r^{1/4}-law fits by 10% in the mean, also with a standard deviation of more than 40%. By comparing the Sersic r_{1/2} with those derived from the bulge-plus-disk fitting, that scatter is also large, at 30%. We conclude that r_{1/2} is generally measured with a typical accuracy of 30-40%. The large uncertainties in r_{1/2} do not impact the fundamental plane analysis because the combination r<I>^{0.76}, which enters the fundamental plane, is extremely stable. The rms scatter in r<I>^{0.76} is less than 3%, regardless of the form of the profile fit to the galaxies. We find that the median bulge fraction of the sample is 84% and that the few E+A galaxies in this sample have disks which make up about 10-35% of their total light. These results are consistent with residuals from fitting 2D r^{1/4}-law models directly to the galaxies, in which disk-like structures are revealed in about half of the sample. Two of the three E+A galaxies show spiral arm structure.
27 pages, 8 figures (2 jpg); abridged abstract; accepted by ApJ on 1 November 1999
References in corpus (3)
- The Evolution of Early-Type Galaxies in Distant Clusters II: Internal Kinematics of 55 Galaxies in the z=0.33 Cluster CL1358+62
- The Evolution of Early-Type Galaxies in Distant Clusters III.: M/L_V Ratios in the z=0.33 Cluster CL1358+62
- The Extragalactic Distance Scale Key Project XXVII. A Derivation of the Hubble Constant Using the Fundamental Plane and Dn-Sigma Relations in Leo I, Virgo, and Fornax
Cited by in corpus (64)
- The epochs of early-type galaxy formation as a function of environment
- The Sloan Lens ACS Survey. V. The Full ACS Strong-Lens Sample
- Massive Dark-matter halos and Evolution of Early-type Galaxies to z=1
- The Fundamental Scaling Relations of Elliptical Galaxies
- The Assembly History of Field Spheroidals: Evolution of Mass-to-light Ratios and Signatures of Recent Star Formation
- The Structure and Dynamics of Luminous and Dark Matter in the Early-Type Lens Galaxy of 0047-281 at z=0.485
- The Evolution of Early-Type Galaxies in Distant Clusters II: Internal Kinematics of 55 Galaxies in the z=0.33 Cluster CL1358+62
- Evolution Since z=1 of the Morphology-density Relation of Galaxies
- Weak homology of elliptical galaxies
- On the estimation of galaxy structural parameters: the Sersic Model
- The Evolution of Early-Type Galaxies in Distant Clusters III.: M/L_V Ratios in the z=0.33 Cluster CL1358+62
- Identifying Lenses with Small-Scale Structure. I. Cusp Lenses
- On the Reported Death of the MACHO Era
- The Detailed Evolution of E+A Galaxies into Early Types
- The Star Formation Epoch of the Most Massive Early-Type Galaxies
- The Nature of E+A Galaxies in Intermediate Redshift Clusters
- The effects of environment on morphological evolution between 0<z<1.2 in the COSMOS Survey
- ROSAT-SDSS Galaxy Clusters Survey. I. The Catalog and the correlation of X-ray and optical properties
- E+A Galaxies and the Formation of Early Type Galaxies at z~0
- The properties of field elliptical galaxies at intermediate redshift. II: photometry and spectroscopy of an HST selected sample
- The properties of field elliptical galaxies at intermediate redshift. III: the Fundamental Plane and the evolution of stellar populations from z~0.4 to z=0
- Identifying Lenses with Small-Scale Structure. II. Fold Lenses
- The Fundamental Plane of Cluster Ellipticals at z = 1.25
- The detailed Fundamental Plane of two high redshift clusters: MS 2053-04 at z=0.58 and MS 1054-03 at z=0.83
- Mass-Selection and the Evolution of the Morphology-Density Relation from z=0.8 to z=0
- A Wide-field Hubble Space Telescope Survey of the Cluster Cl 0024+16 at z=0.4. III: Spectroscopic Signatures of Environmental Evolution in Early Type Galaxies
- On the Assembly History of Early-Type Galaxies in the Hubble Deep Field North
- An X-ray Selected Galaxy Cluster at z=1.11 in the Rosat Deep Cluster Survey
- SPIDER II - The Fundamental Plane of Early-type Galaxies in grizYJHK
- Line Strengths in Early-Type Cluster Galaxies at z=0.33: Implications for alpha/Fe, Nitrogen and the Histories of E/S0s
- Recurring Planetary Debris Transits and Circumstellar Gas around White Dwarf ZTF J03281219
- The Photometric Plane of Elliptical Galaxies
- The Evolution of Balmer Absorption Line Strengths in E/S0 Galaxies from z=0 to z=0.83
- M/L and Color Evolution for A Deep Sample of M* Cluster Galaxies at z~1: The Formation Epoch and the Tilt of the Fundamental Plane
- The SDSS-UKIDSS Fundamental Plane of Early-type Galaxies
- SPIDER - VI. The Central Dark Matter Content of Luminous Early-Type Galaxies: Benchmark Correlations with Mass, Structural Parameters and Environment
- On the evolutionary status of early-type galaxies in clusters at z~0.2 - I. The Fundamental Plane
- An Ultra Metal-poor Star Near the Hydrogen-burning Limit
- Evolution in the Cluster Early-type Galaxy Size-Surface Brightness Relation at z =~ 1
- Sloshing in its cD halo: MUSE kinematics of the central galaxy NGC 3311
- The Kormendy Relation for early-type galaxies. Dependence on the magnitude range
- Optical and Near-Infrared Photometry of Distant Galaxy Clusters
- Morphologies and stellar populations of galaxies in the core of Abell 2218
- Optical and Near-Infrared Structural Properties of Cluster Galaxies at
- The Evolutionary History of Galactic Bulges: Photometric and Spectroscopic Studies of Distant Spheroids in the GOODS Fields
- The low-luminosity galaxy population in the NGC 5044 Group
- Crowded Field Galaxy Photometry: Precision Colors in the CLASH Clusters
- Strong-Lensing Analysis of MS 1358.4+6245: New Multiple Images and Implications for the Well-Resolved z=4.92 Galaxy
- Discs in early-type lensing galaxies: effects on magnification ratios and measurements of
- Looking at the Fundamental Plane through a gravitational lens
- CL 1358+62: Characterizing the Physical Properties of Cluster Galaxies at z=0.33
- Photometric Scaling Relations for Bulges of Galaxies
- A Compact Cluster of Massive Red Galaxies at a Redshift of 1.51
- High-precision abundances of first population stars in NGC 2808: confirmation of a metallicity spread
- The hybrid solution for the Fundamental Plane
- Lensing effects of misaligned disks in dark matter halos
- The Gemini/HST Cluster Project: Structural and Photometric Properties of Galaxies in Three z =0.28-0.89 Clusters
- The Gravitational Lens CFRS03.1077
- A photometric analysis of Abell 1689: two-dimensional multi-structure decomposition, morphological classification, and the Fundamental Plane
- Chemical Tagging N-rich Field Stars with High-resolution Spectroscopy
- Efficiency tests for estimating the gas and stellar population parameters in Type 2 objects
- The Origins of Young Stars in the Direction of the Leading Arm of the Magellanic Stream: Abundances, Kinematics, and Orbits
- TOI-2005b: An Eccentric Warm Jupiter in Spin-Orbit Alignment
- Stellar Abundances at the Center of Early Type Galaxies with Fine Structure