Optical ( VRI ) Photometry in the Field of the Galaxy Cluster AC 118 at z = 0 . 31 ⋆
نویسندگان
چکیده
We present new photometric V-, R-and I-band data for the rich galaxy cluster AC 118 at z = 0.31. The new photometry covers an area of 8.6×8.6 arcmin 2 , corresponding to 2.9×2.9 Mpc 2 (H0 = 50 km s −1 Mpc −1 , q0 = 0.5 and Λ = 0). The data have been collected for a project aimed at studying galaxy evolution through the color-magnitude relation and the fundamental plane. We provide a catalogue including all the sources (N = 1219) detected in the cluster field. The galaxy sample is complete to V = 22.8 mag (N gal = 569), R = 22.3 mag (N gal = 669) and I = 20.8 mag (N gal = 425). We give aperture magnitudes within a fixed aperture of 4.4 arcsec and Kron magnitudes. We also give photo-metric redshifts for 489 sources for which additional U-and K-band photometry is available. We derive and discuss the V-and R-band luminosity functions. The catalogue, which is distributed in electronic form, is intended as a tool for studies in galaxy evolution.
منابع مشابه
The Colour - Magnitude Relation and the Age of Galaxies in the Cluster AC 118 at z = 0 . 31
We derive the Colour-Magnitude (CM) relation for the galaxy cluster AC118 at z=0.31 and use this relation to set constraints on the formation epoch and on the age spread of cluster galaxies in the framework of the passive evolution scenario. This work is based on observations at ESO NTT (OAC guaranteed time). The galaxy population in the core of AC118 was already analyzed by Stan-ford et al. (1...
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We investigate the color-magnitude distribution in the rich cluster AC 118 at z = 0.31. The sample is selected by the photometric redshift technique, allowing to study a wide range of properties of stellar populations, and is complete in the K-band, allowing to study these properties up to a given galaxy mass. We use galaxy templates based on population synthesis models to translate the physica...
متن کاملJ . Age , Metallicity and Star Formation History of Cluster Galaxies
We investigate the color-magnitude distribution in the rich cluster AC 118 at z = 0.31. The sample is selected by the photometric redshift technique, allowing to study a wide range of properties of stellar populations, and is complete in the K-band, allowing to study these properties up to a given galaxy mass. We use galaxy templates based on population synthesis models to translate the physica...
متن کاملJ . Age , Metallicity and Star Formation History of Cluster
We investigate the color-magnitude distribution in the rich cluster AC 118 at z = 0.31. The sample is selected by the photometric redshift technique, allowing to study a wide range of properties of stellar populations, and is complete in the K-band, allowing to study these properties up to a given galaxy mass. We use galaxy templates based on population synthesis models to translate the physica...
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