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20062026
most citedThe Gemini Planet Imager Exoplanet Survey: Giant Planet and Brown Dwarf Demographics From 10-100 AU

476 citations · 1.9k across the 42 of their papers we have counts for

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Showing 2021Show all

8 papers · 1 filter

astro-ph.GA2021★ 12 cited

Stellar feedback in a clumpy galaxy at 3.4

E. Iani, A. Zanella, J. Vernet +18

Giant star-forming regions (clumps) are widespread features of galaxies at . Theory predicts that they can play a crucial role in galaxy evolution if they survive to…

astro-ph.GA2021

No strong dependence of Lyman continuum leakage on physical properties of star-forming galaxies at

A. Saxena, L. Pentericci, R. S. Ellis +15

We present Lyman continuum (LyC) radiation escape fraction measurements for 183 spectroscopically confirmed star-forming galaxies in the redshift range $3.11 < z < 3…

astro-ph.GA2021

The VANDELS survey: global properties of CIII]1908Å 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.GA2021★ 2 cited

An ACA 1mm survey of HzRGs in the ELAIS-S1: survey description and first results

Hugo Messias, Evanthia Hatziminaoglou, Pascale Hibon +16

Radio-emitting jets might be one of the main ingredients shaping the evolution of massive galaxies in the Universe since early cosmic times. However, identifying early radio active…

astro-ph.GA2021

The evolution of the mass-metallicity relations from the VANDELS survey and the GAEA Semi-Analytic model

Fabio Fontanot, Antonello Calabrò, Margherita Talia +18

In this work, we study the evolution of the mass-metallicity relations (MZRs) as predicted by the GAlaxy Evolution and Assembly (GAEA) semi-analytic model. We contrast these predic…

astro-ph.CO2021

The less and the more IGM transmitted galaxies from z~2.7 to z~6 from VANDELS and VUDS

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

Aim. Our aim is to analyse the variance of the Inter-Galactic Medium transmission (IGM) by studying this parameter in the rest-frame UV spectra of a large sample of high redshift g…