The Evolution of the Star Formation of zCOSMOS and SDSS galaxies at z<0.7 as a Function of Mass and Structural Parameters
C. Maier (1), S. J. Lilly (1), G. Zamorani, M. Scodeggio, F., Lamareille, T. Contini, M. T. Sargent, C. Scarlata, P. Oesch (1), C. M., Carollo (1), and zCOSMOS Team ((1) ETH Zurich)

TL;DR
This study compares the evolution of specific star formation rates in massive galaxies at z<0.7, analyzing how they relate to structural parameters like surface mass density and Sersic index, using data from zCOSMOS and SDSS.
Contribution
It provides a comparative analysis of galaxy star formation evolution as a function of structural parameters at low redshift, using a large, consistent galaxy sample.
Findings
Star formation rates vary with surface mass density.
Structural parameters influence galaxy evolution.
Comparison between high-z and local galaxy samples.
Abstract
We present in these proceedings some preliminary results we have obtained studying the evolution of the specific star formation rate as a function of surface mass density and Sersic indices at z<0.7. These results are based on the consistent comparison of the properties of ~ 650 massive zCOSMOS galaxies in a mass-complete sample at 0.5<z<0.7 with a mass-complete sample of ~ 21500 SDSS local galaxies.
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Taxonomy
TopicsAstronomy and Astrophysical Research · Stellar, planetary, and galactic studies · Galaxies: Formation, Evolution, Phenomena
