Chiara Mazzucchelli

TL;DR: Strong evidence of absorption of the spectrum of the quasar redwards of the Lyman α emission line (the Gunn–Peterson damping wing), as would be expected if a significant amount of the hydrogen in the intergalactic medium surrounding J1342 + 0928 is neutral, and a significant fraction of neutral hydrogen is derived, although the exact fraction depends on the modelling.

TL;DR: In this paper, the Leibniz Prize (DFG) was used for the first time to evaluate the performance of the NSF Telescope System Instrumentation Program (TSIP).

TL;DR: In this article, the authors proposed the Cosmic Dawn project, which used the ESO Telescopes at the La Silla Paranal Observatory (ESO-Paral Observatory).

TL;DR: In this article, the authors presented a survey of the [C II] 158 μm line and underlying far-infrared (FIR) dust continuum emission in a sample of 27 z ≳ 6 quasars using the Atacama Large Millimeter Array (ALMA) at 1^" resolution.

TL;DR: Observations of an emission line of singly ionized carbon in four galaxies at z > 6 that are companions of quasars and estimate star-formation rates in the companions of more than 100 solar masses per year, which can account for the population of massive elliptical galaxies in terms of the density of cosmic space.