Surface photometry of WINGS galaxies with GASPHOT
arXiv:1410.2441 · doi:10.1051/0004-6361/201424307
Abstract
Aims. We present the B-, V- and K-band surface photometry catalogs obtained running the automatic software GASPHOT on galaxies from the WINGS cluster survey having isophotal area larger than 200 pixels. The catalogs can be downloaded at the Centre de Donnees Astronomiques de Strasbourg (CDS). Methods. We outline the GASPHOT performances and compare our surface photometry with that obtained by SExtractor, GALFIT and GIM2D. This analysis is aimed at providing statistical information about the accuracy generally achieved by the softwares for automatic surface photometry of galaxies. Results. For each galaxy and for each photometric band the GASPHOT catalogs provide the parameters of the Sersic law best-fitting the luminosity profiles. They are: the sky coordinates of the galaxy center (R:A:; DEC:), the total magnitude (m), the semi-major axis of the effective isophote (Re), the Sersic index (n), the axis ratio (b=a) and a flag parameter (QFLAG) giving a global indication of the fit quality. The WINGS-GASPHOT database includes 41,463 galaxies in the B-band, 42,275 in the V-band, and 71,687 in the K-band. We find that the bright early-type galaxies have larger Sersic indices and effective radii, as well as redder colors in their center. In general the effective radii increase systematically from the K- to the V- and B-band. Conclusions. The GASPHOT photometry turns out to be in fairly good agreement with the surface photometry obtained by GALFIT and GIM2D, as well as with the aperture photometry provided by SExtractor. The main advantages of GASPHOT with respect to other tools are: (i) the automatic finding of the local PSF; (ii) the short CPU time of execution; (iii) the remarkable stability against the choice of the initial guess parameters. All these characteristics make GASPHOT an ideal tool for blind surface photometry of large galaxy samples in wide-field CCD mosaics.
arXiv comment14 pages, 9 figures
References in corpus (35)
- Detailed Structural Decomposition of Galaxy Images
- NYU-VAGC: a galaxy catalog based on new public surveys
- The Galaxy Luminosity Function and Luminosity Density at Redshift z=0.1
- On the shape of the light profiles of early-type galaxies
- A Catalog of Bulge+Disk Decompositions and Updated Photometry for 1.12 Million Galaxies in the Sloan Digital Sky Survey
- Structural and Photometric Classification of Galaxies - I. Calibration Based on a Nearby Galaxy Sample
- GEMS: Galaxy fitting catalogues and testing parametric galaxy fitting codes
- The Millennium Galaxy Catalogue: Bulge/Disc Decomposition of 10095 Nearby Galaxies
- The Millennium Galaxy Catalogue: 16 < B_MGC < 24 galaxy counts and the calibration of the local galaxy luminosity function
- WINGS: a WIde-field Nearby Galaxy-cluster Survey. I - Optical imaging
- Superdense galaxies and the mass-size relation at low redshift
- Superdense Massive Galaxies in Wings Local Clusters
- A Catalog of Morphological Types in 10 Distant Rich Clusters of Galaxies
- WINGS-SPE Spectroscopy in the WIde-field Nearby Galaxy-cluster Survey
- Galaxy stellar mass functions of different morphological types in clusters, and their evolution between z=0.8 and z=0
- Early-Type Galaxies in the Hubble Deep Field: The Star Formation History
- The evolution of spiral, S0 and elliptical galaxies in clusters
- WINGS: A WIde-field Nearby Galaxy-cluster Survey. II. Deep optical photometry of 77 nearby clusters
- The evolution of the number density of compact galaxies
- WINGS Data Release: a database of galaxies in nearby clusters
- Superdense massive galaxies in the ESO Distant Cluster Survey (EDisCS)
- Morphology of galaxies in the WINGS clusters
- The effect of the environment on the stellar mass - size relation of present-day galaxies
- The Millennium Galaxy Catalogue: The photometric accuracy, completeness and contamination of the 2dFGRS and SDSS-EDR & DR1 datasets
- WINGS-SPE II: A catalog of stellar ages and star formation histories, stellar masses and dust extinction values for local clusters galaxies
- The importance of the local density in shaping the galaxy stellar mass functions
- WINGS: a WIde-field nearby Galaxy-cluster survey III. Deep near-infrared photometry of 28 nearby clusters
- Evolution of BCGs structural parameters in the last 6 Gyr: feedback processes versus merger events
- WINGS-SPE III: Equivalent width measurements, spectral properties and evolution of local cluster galaxies
- The Shapes of BCGs and normal Ellipticals in Nearby Clusters
- The evolution of early-type galaxies in clusters from z~ 0.8 to z~ 0: the ellipticity distribution and the morphological mix
- U-band photometry of 17 WINGS clusters
- The hybrid solution for the Fundamental Plane
- On the connection between shape and stellar population in early-type galaxies
- The evolution of galaxy sizes
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- GASP I: Gas stripping phenomena in galaxies with MUSE
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- OmegaWINGS: OmegaCAM@VST observations of WINGS galaxy clusters
- Morphological Fractions of Galaxies in WINGS Clusters: revisiting the Morphology-Density Paradigm
- OmegaWINGS: The first complete census of post starburst galaxies in clusters in the local universe
- Structural and dynamical modeling of WINGS clusters. I. The distribution of cluster galaxies of different morphological classes within regular and irregular clusters
- Emission Line Galaxies and Active Galactic Nuclei in WINGS clusters
- Characterization of Omega-WINGS galaxy clusters. I. Stellar light and mass profiles
- Shapley Supercluster Survey: Construction of the Photometric Catalogues and i-band Data Release
- The parallelism between galaxy clusters and early-type galaxies: I. The light and mass profiles
- The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship
- Multi-wavelength structure analysis of local cluster galaxies. The WINGS project
- The Fundamental Plane in the hierarchical context
- A Maximum Parsimony analysis of the effect of the environment on the evolution of galaxies
- The scaling relations of galaxies back in time: the road toward virialization
- A new framework for understanding the evolution of early-type galaxies