We present a catalogue of structural parameters for 8814 galaxies in the 25 fields of the Hubble Space Telescope/ACS Coma Treasury Survey. Parameters from Sersic fits to the two-dimensional surface brightness distributions are given for all galaxies from our published Coma photometric catalogue with mean effective surface brightness brighter than 26.0 mag arcsec-2 and brighter than 24.5 mag (equivalent to absolute magnitude -10.5), as given by the fits, all in F814W(AB). The sample comprises a mixture of Coma members and background objects; 424 galaxies have redshifts and of these 163 are confirmed members. The fits were carried out using both the gim2d and galfit codes. We provide the following parameters: galaxy ID, RA, Dec., the total co...
We introduce a new galaxy image decomposition tool, GALPHAT (GALaxy PHotometric ATtributes), to prov...
We present a quantitative morphological analysis of 187 galaxies in a region covering the central 0....
We use ACS data from the HST Treasury survey of the Coma cluster (z˜0.02) to study the properties of...
We present a catalogue of structural parameters for 8814 galaxies in the 25 fields of the Hubble Spa...
We present a catalogue of structural parameters for 8814 galaxies in the 25 fields of the Hubble Spa...
The Coma cluster, Abell 1656, was the target of an HST-ACS Treasury program designed for deep imagin...
The Coma cluster, Abell 1656, was the target of an HST-ACS Treasury program designed for deep imagin...
The Coma cluster, Abell 1656, was the target of an HST-ACS Treasury program designed for deep imagin...
The Coma cluster, Abell 1656, was the target of an HST-ACS Treasury program designed for deep imagin...
We present global structural parameter measurements of 109,533 unique, H-F160W-selected objects from...
We use high-resolution (similar to 0.'' 1) F814W Advanced Camera for Surveys (ACS) images from the H...
We use high-resolution (~0farcs1) F814W Advanced Camera for Surveys (ACS) images from the Hubble Spa...
Using wide-field, two-color Hubble Space Telescope (HST) imaging of the cluster Cl 1358 + 62 (z = 0....
The quantitative morphological classification of distant galaxies is essential to the understanding ...
We use high-resolution (similar to 0.'' 1) F814W Advanced Camera for Surveys (ACS) images ...
We introduce a new galaxy image decomposition tool, GALPHAT (GALaxy PHotometric ATtributes), to prov...
We present a quantitative morphological analysis of 187 galaxies in a region covering the central 0....
We use ACS data from the HST Treasury survey of the Coma cluster (z˜0.02) to study the properties of...
We present a catalogue of structural parameters for 8814 galaxies in the 25 fields of the Hubble Spa...
We present a catalogue of structural parameters for 8814 galaxies in the 25 fields of the Hubble Spa...
The Coma cluster, Abell 1656, was the target of an HST-ACS Treasury program designed for deep imagin...
The Coma cluster, Abell 1656, was the target of an HST-ACS Treasury program designed for deep imagin...
The Coma cluster, Abell 1656, was the target of an HST-ACS Treasury program designed for deep imagin...
The Coma cluster, Abell 1656, was the target of an HST-ACS Treasury program designed for deep imagin...
We present global structural parameter measurements of 109,533 unique, H-F160W-selected objects from...
We use high-resolution (similar to 0.'' 1) F814W Advanced Camera for Surveys (ACS) images from the H...
We use high-resolution (~0farcs1) F814W Advanced Camera for Surveys (ACS) images from the Hubble Spa...
Using wide-field, two-color Hubble Space Telescope (HST) imaging of the cluster Cl 1358 + 62 (z = 0....
The quantitative morphological classification of distant galaxies is essential to the understanding ...
We use high-resolution (similar to 0.'' 1) F814W Advanced Camera for Surveys (ACS) images ...
We introduce a new galaxy image decomposition tool, GALPHAT (GALaxy PHotometric ATtributes), to prov...
We present a quantitative morphological analysis of 187 galaxies in a region covering the central 0....
We use ACS data from the HST Treasury survey of the Coma cluster (z˜0.02) to study the properties of...