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CALIFA, the Calar Alto Legacy Integral Field Area survey : I. Survey presentation
The final product of galaxy evolution through cosmic time is the population of galaxies in the local universe. These galaxies are also those that can be studied in most detail, thus providing a…
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The O3N2 and N2 abundance indicators revisited: improved calibrations based on CALIFA and T e-based literature data
The use of integral field spectroscopy is since recently allowing to measure the emission line fluxes of an increasingly large number of star-forming galaxies, both locally and at high redshift. Many…
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The evolution of the luminosity functions in the FORS deep field from low to high redshift. II. The red bands
Received -; accepted - Abstract. We present the redshift evolution of the restframe galaxy luminosity function (LF) in the red r', i', and z' bands as derived from the FORS Deep Field (FDF), thus…
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The z=2.72 galaxy cB58: a gravitational fold arc lensed by the cluster MS 1512+36
Using HST WFPC2 V- and R-band data of the z=0.37 cluster MS 1512+36, we show that the z=2.72 ‘protogalaxy’ cB58 is not extraordinarily luminous intrinsically but lensed into a gravitational fold arc…
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Mass-metallicity relation explored with CALIFA I. Is there a dependence on the star-formation rate?
We studied the global and local ℳ-Z relation based on the first data available from the CALIFA survey (150 galaxies). This survey provides integral field spectroscopy of the complete optical extent…
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The Tully-Fisher relation at intermediate redshift ⋆,⋆⋆
Using the Very Large Telescope in Multi Object Spectroscopy mode, we have observed a sample of 113 field spiral galaxies in the FORS Deep Field (FDF) with redshifts in the range 0.1< z< 1.0. The…
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Exploring Cluster Elliptical Galaxies as Cosmological Standard Rods
We explore the possibility of calibrating massive cluster elliptical galaxies as cosmological standard rods using the fundamental plane relation combined with a correction for luminosity evolution.…
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CALIFA : a diameter-selected sample for an integral field spectroscopy galaxy survey
We describe and discuss the selection procedure and statistical properties of the galaxy sample used by the Calar Alto Legacy Integral Field Area (CALIFA) survey, a public legacy survey of 600…
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Bar pattern speeds in CALIFA galaxies. I. Fast bars across the Hubble sequence
J.M.A. acknowledges support from the European Research Council Starting Grant (SEDmorph; P.I. V. Wild). Date of Acceptance: 07/01/2015
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The effect of ram pressure on the star formation, mass distribution and morphology of galaxies
Aims. We investigate the dependence of star formation and the distribution of the components of galaxies on the strength of ram pressure. Several mock observations in X-ray, H α and HI wavelength for…
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