368 citations · 2.7k across the 27 of their papers we have counts for
16 papers · 1 filter
The impact of nebular Lyman-Continuum on ionising photons budget and escape fractions from galaxies
C. Simmonds, A. Verhamme, A. K. Inoue +3
Several Lyman Continuum (LyC) emitters have been detected so far, but their observed ionising spectra sometimes differ from attenuated stellar spectra predicted by stellar populati…
The Prevalence of Galaxy Overdensities Around UV-Luminous Lyman Emitters in the Epoch of Reionization
E. Leonova, P. A. Oesch, Y. Qin +19
Before the end of the epoch of reionization, the Hydrogen in the Universe was predominantly neutral. This leads to a strong attenuation of Ly lines of galaxies in th…
The Spitzer/IRAC Legacy over the GOODS Fields: Full-Depth 3.6, 4.5, 5.8 and 8.0um Mosaics and Photometry for > 9000 Galaxies at z~3.5-10 from the GOODS Re-ionization Era wide-Area Treasury from Spitzer (GREATS)
Mauro Stefanon, Ivo Labbé, Pascal A. Oesch +9
We present the deepest Spitzer/IRAC , , and m wide-area mosaics yet over the GOODS-N and GOODS-S fields as part of the GOODS Re-ionization Era wide-Area Treas…
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…
Optical Line Emission from z6.8 Sources with Deep Constraints on Ly Visibility
M. Castellano, L. Pentericci, A. Fontana +15
We analyze a sample of -dropout galaxies in the CANDELS GOODS South and UDS fields that have been targeted by a dedicated spectroscopic campaign aimed at detecting their Ly l…
Magnifying the early episodes of star formation: super star clusters at cosmological distances
E. Vanzella, M. Castellano, M. Meneghetti +27
We study the spectrophotometric properties of a highly magnified (μ~40-70) pair of stellar systems identified at z=3.2222 behind the Hubble Frontier Field galaxy cluster MACS~J0416…
Characterization of star-forming dwarf galaxies at 0.1 0.9 in VUDS: Probing the low-mass end of the mass-metallicity relation
A. Calabrò, R. Amorín, A. Fontana +19
We present the discovery and spectrophotometric characterization of a large sample of 164 faint ( - mag) star-forming dwarf galaxies (SFDGs) at redshift $0.1…
Analogs of primeval galaxies two billion years after the Big Bang
Ricardo Amorín, A. Fontana, E. Pérez-Montero +30
Deep observations are revealing a growing number of young galaxies in the first billion year of cosmic time. Compared to typical galaxies at later times, they show more extreme emi…
Paving the way for the JWST: witnessing globular cluster formation at z>3
E. Vanzella, F. Calura, M. Meneghetti +17
We report on five compact, extremely young (<10Myr) and blue (β_UV<-2.5, F_λ=λ^β) objects observed with VLT/MUSE at redshift 3.1169, 3.235, in addition to three objects at z=6.145.…
Illuminating gas in-/outflows in the MUSE deepest fields: discovery of Ly-alpha nebulae around forming galaxies at z~3.3
E. Vanzella, I. Balestra, M. Gronke +11
We report on the discovery of extended Ly-alpha nebulae at z~3.3 in the Hubble Ultra Deep Field (HUDF, ~ 40 kpc X 80 kpc) and behind the Hubble Frontier Fields galaxy cluster MACSJ…
Hubble imaging of the ionizing radiation from a star-forming galaxy at z=3.2 with fesc>50%
E. Vanzella, S. de Barros, K. Vasei +20
Star-forming galaxies are considered to be the leading candidate sources that dominate the cosmic reionization at z>7, and the search for analogs at moderate redshift showing Lyman…
A Coherent Study of Emission Lines from Broad-Band Photometry: Specific Star-Formation Rates and [OIII]/Hβ Ratio at 3 < z < 6
A. L. Faisst, P. Capak, B. C. Hsieh +14
We measure the Hα and [OIII] emission line properties as well as specific star-formation rates (sSFR) of spectroscopically confirmed 3<z<6 galaxies in COSMOS from their observed co…
Limits on the LyC signal from z~3 sources with secure redshift and HST coverage in the E-CDFS field
L. Guaita, L. Pentericci, A. Grazian +23
Aim: We aim to measure the LyC signal from a sample of sources in the Chandra deep field south. We collect star-forming galaxies (SFGs) and active galactic nuclei (AGN) with accura…
Dust attenuation of the nebular regions and optical emission lines of star-forming galaxies
S. de Barros, N. Reddy, I. Shivaei
We use a sample of 149 spectroscopically confirmed UV-selected galaxies at to investigate the relative dust attenuation of the stellar continuum and the nebular emission…
An extreme [OIII] emitter at : a low metallicity Lyman continuum source
S. de Barros, E. Vanzella, R. Amorín +16
[Abridged] We investigate the physical properties of a Lyman continuum emitter candidate at with photometric coverage from to MIPS 24m band and VIMOS/VLT and MOSFI…
A Study of Massive and Evolved Galaxies at High Redshift
Hooshang Nayyeri, Bahram Mobasher, Shoubaneh Hemmati +14
We use data taken as part of HST/WFC3 observations of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) to identify massive and evolved galaxies at 3<z<4…