C. Mancini

TL;DR: In this article, the authors studied the properties of giant star-forming clumps in five z ~ 2 star forming disks with deep SINFONI AO spectroscopy at the ESO VLT.

TL;DR: In this paper, the authors exploit deep observations of the GOODS-N field taken with PACS onboard of Herschel, as part of the PACS evolutionary probe guaranteed time (PEP), to study the link between star formation and stellar mass in galaxies to z ~ 2.

TL;DR: In this paper, the authors presented a new near-infrared survey covering the 2 deg^2 COSMOS field conducted using WIRCam at the Canada-France-Hawaii Telescope.

TL;DR: Mapping star-forming activity and densities shows an evolutionary connection between galaxies at z ~ 2.2 and those 10 million years later, and it is found that, in the most massive galaxies, star formation is quenched from the inside out, on time scales less than 1 billion years in the inner regions, up to a few billion Years in the outer disks.

TL;DR: In this paper, the radial distributions of Hα surface brightness, stellar mass surface density, and dynamical mass at 2 kpc resolution in 19 z ∼ 2 star-forming disks with deep SINFONI adaptive optics spectroscopy at the ESO Very Large Telescope were derived.