353 citations · 10.1k across the 134 of their papers we have counts for
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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…
An environmental dependence of the physical and structural properties in the Hydra Cluster galaxies
Ciria Lima-Dias, Antonela Monachesi, Sergio Torres-Flores +20
The nearby Hydra Cluster (50 Mpc) is an ideal laboratory to understand, in detail, the influence of the environment on the morphology and quenching of galaxies in dense envir…
Reconciling escape fractions and observed line emission in Lyman-continuum-leaking galaxies
L. Ramambason, D. Schaerer, G. Stasińska +5
Finding and elucidating the properties of Lyman-continuum(LyC)-emitting galaxies is an important step for our understanding of cosmic reionization. Although the z - 0.3-0.4 LyC emi…
The spectroscopic follow-up of the QUBRICS bright quasar survey
K. Boutsia, A. Grazian, G. Calderone +11
We present the results of the spectroscopic follow up of the QUBRICS survey. The selection method is based on a machine learning approach applied to photometric catalogs, covering…
The VANDELS survey: Discovery of massive overdensities of galaxies at z>2
L. Guaita, E. Pompei, M. Castellano +19
We want to investigate whether we can use Lyalpha emission to obtain information on the environment properties and whether Lyalpha emitters show different characteristics as a func…
The ALPINE-ALMA [CII] Survey: Obscured Star Formation Rate Density and Main Sequence of star-forming galaxies at z>4
Y. Khusanova, M. Béthermin, O. Le Fèvre +30
Star formation rate (SFR) measurements at z>4 have relied mostly on rest-frame far-ultraviolet (FUV) observations. The corrections for dust attenuation based on IRX- relation ar…
The ALPINE-ALMA [CII] survey: Molecular gas budget in the Early Universe as traced by [CII]
M. Dessauges-Zavadsky, M. Ginolfi, F. Pozzi +32
The molecular gas content of normal galaxies at z>4 is poorly constrained, because the commonly used molecular gas tracers become hard to detect. We use the [CII]158um luminosity,…
The ALPINE-ALMA [CII] survey: Dust attenuation properties and obscured star formation at z~4.4-5.8
Yoshinobu Fudamoto, P. A. Oesch, A. Faisst +34
We present dust attenuation properties of spectroscopically confirmed star forming galaxies on the main sequence at a redshift of ~4.4-5.8. Our analyses are based on the far infrar…
X-ray properties of He II 1640 emitting galaxies in VANDELS
A. Saxena, L. Pentericci, D. Schaerer +13
We explore X-ray emission from a sample of 18 He II 1640 emitting star-forming galaxies at z ~ 2.3-3.6 from the VANDELS survey in the Chandra Deep Field South, to set constraints o…
The ALPINE-ALMA [CII] Survey: Size of Individual Star-Forming Galaxies at z=4-6 and their Extended Halo Structure
S. Fujimoto, J. D. Silverman, Matthieu Bethermin +31
We present the physical extent of [CII] 158um line-emitting gas from 46 star-forming galaxies at z=4-6 from the ALMA Large Program to INvestigate CII at Early Times (ALPINE). Using…
The role of galaxy mass on AGN emission: a view from the VANDELS survey
M. Magliocchetti, L. Pentericci, M. Cirasuolo +13
We present a comparative analysis of the properties of AGN emitting at radio and X-ray wavelengths. The study is performed on 907 X-ray AGN and 100 radio AGN selected on the CDFS a…
The ALPINE-ALMA [CII] survey. Little to no evolution in the [CII]-SFR relation over the last 13 Gyr
D. Schaerer, M. Ginolfi, M. Bethermin +34
The [CII] 158 micron line is one of the strongest IR emission lines, which has been shown to trace the star-formation rate (SFR) of galaxies in the nearby Universe and up to $z \si…
The ALPINE-ALMA [CII] Survey: data processing, catalogs, and statistical source properties
M. Bethermin, Y. Fudamoto, M. Ginolfi +33
The ALPINE-ALMA large program targets the [CII] 158 m line and the far-infrared continuum in 118 spectroscopically confirmed star-forming galaxies between z=4.4 and z=5.9. It re…
Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5
A. C. Carnall, S. Walker, R. J. McLure +19
We present a sample of 151 massive () quiescent galaxies at , based on a sophisticated Bayesian spectral energy distribution fitting analy…