Paolo Saracco

TL;DR: In this article, a detailed analysis of the stellar mass content of galaxies up to as obtained from the K20-spectrophotometric galaxy sample is presented, where a Maximal Age approach is used to obtain the maximal mass compatible with the observed color, and a Best Fit model, where the best fitting spectrum to the complete multicolor distribution is used.

TL;DR: The optical rest-frame sizes of 10 of the most massive (∼5 × 10 11 h −2 M� ) galaxies found in the near-infrared MUNICS survey at 1.2 < z < 1.7 are analyzed in this article.

TL;DR: In this article, a detailed analysis of the stellar mass content of galaxies up to z = 2.5 in the K20 galaxy sample is presented, which has a 92% spectroscopic completeness and a complete $UBVRIzJK_s$ multicolor coverage.

TL;DR: In this article, the results of VLT optical spectroscopy of a complete sample of 78 EROs with over a field of 52 arcmin2 were presented and discussed the average spectrum.

TL;DR: The K20 survey as mentioned in this paper is the most complete near infrared-selected, deep (Ks < 20) redshift survey targeting galaxies in two independent regions of the sky, the Chandra Deep Field South and the field around the quasar.