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Kiloparsec-scale gaseous clumps and star formation at
S. Carniani, R. Maiolino, R. Amorin +13
We investigate the morphology of the [CII] emission in a sample of "normal" star-forming galaxies at in relation to their UV (rest-frame) counterpart. We use new ALMA obs…
On the faint-end of the galaxy luminosity function in the Epoch of Reionization: updated constraints from the HST Frontier Fields
B. Yue, M. Castellano, A. Ferrara +12
Ultra-faint galaxies are hosted by small dark matter halos with shallow gravitational potential wells, hence their star formation activity is more sensitive to feedback effects. Th…
A VLT/FORS2 view at : Lyman- emitter fraction and galaxy physical properties at the edge of the epoch of cosmic reionization
S. De Barros, L. Pentericci, E. Vanzella +10
The fraction of Lyman- emitters among the galaxy population has been found to increase from to and drop dramatically at . This drop has been interpreted a…
Ly-Lyman Continuum connection in 3.5 < z < 4.3 star-forming galaxies from the VUDS survey
F. Marchi, L. Pentericci, L. Guaita +16
To identify the galaxies responsible for the reionization of the Universe, we must rely on the investigation of the Lyman Continuum (LyC) properties of z<5 star-forming galaxies, w…
The VIMOS Ultra Deep Survey: Nature, ISM properties, and ionizing spectra of CIII]1909 emitters at z=2-4
K. Nakajima, D. Schaerer, O. Le Fevre +12
Context: Ultraviolet (UV) emission-line spectra are used to spectroscopically confirm high-z galaxies and increasingly also to determine their physical properties. Aims: To interpr…
Chasing passive galaxies in the early Universe: a critical analysis in CANDELS GOODS-South
E. Merlin, A. Fontana, M. Castellano +12
We search for passive galaxies at in the GOODS-South field, using different techniques based on photometric data, and paying attention to develop methods that are sensitive t…