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Cited article:

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The ESO-Sculptor Survey: Evolution of late-type galaxies at redshifts 0.1–0.5

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The Munich Near‐Infrared Cluster Survey (MUNICS). VI. The Stellar Masses ofK‐Band–selected Field Galaxies toz ∼ 1.2

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The environmental dependence of the relations between stellar mass, structure, star formation and nuclear activity in galaxies

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A Physical Model for the Coevolution of QSOs and Their Spheroidal Hosts

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Near-Infrared Bright Galaxies at z 2. Entering the Spheroid Formation Epoch?

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K$_{\mbox{\fontsize{12pt}{14pt}\selectfont{\textit{s}}}}$-band luminosity function of thez= 1.237 cluster of galaxies RDCS J1252.9-2927

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The Cosmic Evolution of the Galaxy Luminosity Density

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