activity
19942023
most citedThe VIMOS Ultra-Deep Survey: ~10,000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2<z<~6

353 citations · 8.2k across the 93 of their papers we have counts for

collaborators
Showing 2010Show all

7 papers · 1 filter

astro-ph.CO2010★ 65 cited

A critical analysis of the UV Luminosity Function at redshift~7 from deep WFC3 data

A. Grazian, M. Castellano, A. M. Koekemoer +7

The study of the Luminosity Function (LF) of Lyman Break Galaxies (LBGs) at z=7 is important for ascertaining their role in the reionization of the Universe. We perform a detailed…

astro-ph.CO2010★ 184 cited

Spectroscopic confirmation of two Lyman break galaxies at redshift beyond 7

E. Vanzella, L. Pentericci, A. Fontana +12

We report the spectroscopic confirmation of two Lyman break galaxies at redshift > 7. The galaxies were observed as part of an ultra-deep spectroscopic campaign with FORS2 at the E…

astro-ph.CO2010★ 160 cited

The lack of intense Lyman~alpha in ultradeep spectra of z=7 candidates in GOODS-S: imprint of reionization?

A. Fontana, E. Vanzella, L. Pentericci +10

We present ultradeep optical spectroscopy obtained with FORS2 on VLT of seven Lyman-break galaxy (LBG) candidates at z>6.5 selected in the GOODS-S field from Hawk-I/VLT and WFC3/HS…

astro-ph.CO2010★ 82 cited

The bright end of the z ~ 7 UV Luminosity Function from a wide and deep HAWK-I survey

M. Castellano, A. Fontana, D. Paris +23

(Abridged) We present here the second half of an ESO Large Programme, which exploits the unique combination of area and sensitivity provided in the near-IR by the camera Hawk-I at…

astro-ph.CO2010★ 100 cited

The dust content of high-z submillimeter galaxies revealed by Herschel

P. Santini, R. Maiolino, B. Magnelli +38

We use deep observations taken with the Photodetector Array Camera and Spectrometer (PACS), on board the Herschel satellite as part of the PACS evolutionary probe (PEP) guaranteed…

astro-ph.CO2010★ 50 cited

Physical and morphological properties of z~3 LBGs: dependence on Lyalpha line emission

L. Pentericci, A. Grazian, C. Scarlata +4

We investigate the physical and morphological properties of LBGs at z ~2.5 to ~3.5, to determine if and how they depend on the nature and strength of the Lyalpha emission. We selec…