papers

Publications (22)

astro-ph.GA2019

The VANDELS survey: the star-formation histories of massive quiescent galaxies at 1.0 < z < 1.3

A. C. Carnall, R. J. McLure, J. S. Dunlop +19

We present a Bayesian full-spectral-fitting analysis of 75 massive () UVJ-selected galaxies at redshifts of , combining extremely deep rest-…

astro-ph.GA2018

CANDELSz7: a large spectroscopic survey of CANDELS galaxies in the reionization epoch

L. Pentericci, E. Vanzella, M. Castellano +15

We present the results of CANDELSz7, an ESO large program aimed at confirming spectroscopically a homogeneous sample of z~6 and z~7 star forming galaxies. The candidates were selec…

astro-ph.GA2019

The VANDELS survey: the stellar metallicities of star-forming galaxies at 2.5 < z < 5.0

F. Cullen, R. J. McLure, J. S. Dunlop +24

We present the results of a study utilising ultra-deep, rest-frame UV, spectroscopy to quantify the relationship between stellar mass and stellar metallicity for 681 star-forming g…

astro-ph.GA2018

The VANDELS survey: Dust attenuation in star-forming galaxies at

F. Cullen, R. J. McLure, S. Khochfar +15

We present the results of a new study of dust attenuation at redshifts based on a sample of star-forming galaxies from the VANDELS spectroscopic survey. Motivated…

astro-ph.GA2018

The VANDELS ESO public spectroscopic survey: observations and first data release

L. Pentericci, R. J. McLure B. Garilli, O. Cucciati +93

This paper describes the observations and the first data release (DR1) of the ESO public spectroscopic survey "VANDELS, a deep VIMOS survey of the CANDELS CDFS and UDS fields". VAN…

astro-ph.GA2018

The VANDELS ESO public spectroscopic survey

R. J. McLure, L. Pentericci, A. Cimatti +92

VANDELS is a uniquely-deep spectroscopic survey of high-redshift galaxies with the VIMOS spectrograph on ESO's Very Large Telescope (VLT). The survey has obtained ultra-deep optica…

astro-ph.GA2018

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…

astro-ph.GA2018

Discovery of a radio galaxy at z = 5.72

A. Saxena, M. Marinello, R. A. Overzier +11

We report the discovery of the most distant radio galaxy to date, TGSS1530 at a redshift of close to the presumed end of the Epoch of Reionisation. The radio galaxy was se…

astro-ph.GA2017

New constraints on the average escape fraction of Lyman continuum radiation in z~4 galaxies from the VIMOS Ultra Deep Survey (VUDS)

F. Marchi, L. Pentericci, L. Guaita +20

Determining the average fraction of Lyman continuum (LyC) photons escaping high redshift galaxies is essential for understanding how reionization proceeded in the z>6 Universe. We…

astro-ph.GA2017

The VIMOS Ultra-Deep Survey: evidence for AGN feedback in galaxies with CIII]-1908Ã ~emission 10.8 to 12.5 Gyr ago

O. Le Fèvre, B. C. Lemaux, K. Nakajima +19

We analyze the CIII]-1908Ã emission properties in a sample of 3899 star-forming galaxies (SFGs) at 2<z<3.8 from the VIMOS Ultra-Deep Survey (VUDS). We find a median EW(CIII])=2.0$\…

astro-ph.GA2018

Spectroscopic investigation of a reionized galaxy overdensity at z=7

M. Castellano, L. Pentericci, E. Vanzella +17

We present deep spectroscopic follow-up observations of the Bremer Deep Field (BDF) where the two 7 bright Ly emitters (LAE) BDF521 and BDF3299 were previously discovere…

astro-ph.GA2017

The Lyman Continuum escape fraction of faint galaxies at z~3.3 in the CANDELS/GOODS-North, EGS, and COSMOS fields with LBC

A. Grazian, E. Giallongo, D. Paris +41

The reionization of the Universe is one of the most important topics of present day astrophysical research. The most plausible candidates for the reionization process are star-form…

astro-ph.GA2021

The VANDELS survey: global properties of CIII]1908Ã emitting star-forming galaxies at z3

M. Llerena, R. Amorín, F. Cullen +17

We study the mean properties of a large representative sample of 217 galaxies showing CIII] emission at , selected from a parent sample of 750 main-sequence star-formi…

astro-ph.GA2020

The VANDELS survey: the relation between UV continuum slope and stellar metallicity in star-forming galaxies at z~3

A. Calabrò, M. Castellano, L. Pentericci +23

The estimate of stellar metallicities (Z*) of high-z galaxies are of paramount importance in order to understand the complexity of dust effects and the reciprocal interrelations am…

astro-ph.GA2019

The UV and Ly Luminosity Functions of galaxies and the Star Formation Rate Density at the end of HI reionization from the VIMOS Ultra-Deep Survey (VUDS)

Y. Khusanova, O. Le Fèvre, P. Cassata +25

We establish a robust statistical description of the star-forming galaxy population at the end of cosmic HI reionization () from a large sample of 52 galaxies with…

astro-ph.SR2015

B.R.N.O. Contributions #39 Times of minima

K. Hoňková, J. Juryšek, M. Lehký +43

This paper presents 1463 times of minima for 455 objects acquired by 46 members and cooperating observers of the Variable Star and Exoplanet Section of the Czech Astronomical Socie…

astro-ph.GA2019

The VANDELS survey: the role of ISM and galaxy physical properties on the escape of Lyα emission in z 3.5 star-forming galaxies

F. Marchi, L. Pentericci, L. Guaita +20

We investigate the physical properties of a sample of 52 Lyα emitting galaxies in the VANDELS survey, with particular focus on the role of kinematics and neutral hydrogen column d…

astro-ph.GA2020

The properties of He II 1640 emitters at z ~ 2.5-5 from the VANDELS survey

A. Saxena, L. Pentericci, M. Mirabelli +24

Strong He II emission is produced by low-metallicity stellar populations. Here, we aim to identify and study a sample of He II -emitting galaxies at redshifts of $z \sim 2.…

astro-ph.GA2023

The VANDELS ESO public spectroscopic survey: The spectroscopic measurements catalogue

M. Talia, C. Schreiber, B. Garilli +36

VANDELS is a deep spectroscopic survey, performed with the VIMOS instrument at VLT, aimed at studying in detail the physical properties of high-redshift galaxies. VANDELS targeted…

physics.flu-dyn2009

Viscous cavity damping of a microlever in a simple fluid

A. Siria, A. Drezet, F. Marchi +3

We consider the problem of oscillation damping in air of a thermally actuated microlever as it is gradually approached towards an infinite wall in parallel geometry. As the gap is…

astro-ph.GA2017

The VIMOS Ultra Deep Survey: The role of HI kinematics and HI column density on the escape of Lyalpha photons in star-forming galaxies at 2<z<4

L. Guaita, M. Talia, L. Pentericci +22

We selected a sample of 76 Lya emitting galaxies from the VIMOS Ultra Deep Survey (VUDS) at 2<z<4. We estimated the velocity of the neutral gas flowing out of the interstellar medi…

astro-ph.CO2019

The Intergalactic medium transmission towards z>4 galaxies with VANDELS and the impact of dust attenuation

R. Thomas, L. Pentericci, O. Le Fèvre +22

Aims. Our aim is to estimate the intergalactic medium transmission towards UV-selected star-forming galaxies at redshift 4 and above and study the effect of the dust attenuation on…