The GLASS-JWST early release science program. I. Survey design and release plans
T Treu, G Roberts-Borsani, M Bradac… - The Astrophysical …, 2022 - iopscience.iop.org
Abstract The GLASS-JWST Early Release Science (hereafter GLASS-JWST-ERS) Program
will obtain and make publicly available the deepest extragalactic data of the ERS campaign …
will obtain and make publicly available the deepest extragalactic data of the ERS campaign …
JWST UNCOVER: extremely Red and Compact Object at z phot≃ 7.6 triply imaged by A2744
LJ Furtak, A Zitrin, A Plat, S Fujimoto… - The Astrophysical …, 2023 - iopscience.iop.org
Recent JWST/NIRCam imaging taken for the ultra-deep UNCOVER program reveals a very
red dropout object at z phot≃ 7.6, triply imaged by the galaxy cluster A2744 (zd= 0.308). All …
red dropout object at z phot≃ 7.6, triply imaged by the galaxy cluster A2744 (zd= 0.308). All …
Probing the faint-end luminosity function of Lyman-alpha emitters at 3< z< 7 behind 17 MUSE lensing clusters
Context. This paper presents a study of the galaxy Lyman-alpha luminosity function (LF)
using a large sample of 17 lensing clusters observed by the Multi Unit Spectroscopic …
using a large sample of 17 lensing clusters observed by the Multi Unit Spectroscopic …
Most of the photons that reionized the Universe came from dwarf galaxies
The identification of sources driving cosmic reionization, a major phase transition from
neutral hydrogen to ionized plasma around 600–800 Myr after the Big Bang,–, has been a …
neutral hydrogen to ionized plasma around 600–800 Myr after the Big Bang,–, has been a …
Closing in on the sources of cosmic reionization: First results from the GLASS-JWST program
S Mascia, L Pentericci, A Calabrò, T Treu… - Astronomy & …, 2023 - aanda.org
The escape fraction of Lyman-continuum (LyC) photons (f esc) is a key parameter for
determining the sources of cosmic reionization at z≥ 6. At these redshifts, owing to the …
determining the sources of cosmic reionization at z≥ 6. At these redshifts, owing to the …
z∼ 2–9 galaxies magnified by the Hubble Frontier Field clusters. II. Luminosity functions and constraints on a faint-end turnover
RJ Bouwens, G Illingworth, RS Ellis… - The Astrophysical …, 2022 - iopscience.iop.org
We present new determinations of the rest-UV luminosity functions (LFs) at z= 2–9 to
extremely low luminosities (>− 14 mag) from a sample of> 2500 lensed galaxies found …
extremely low luminosities (>− 14 mag) from a sample of> 2500 lensed galaxies found …
UNCOVERing the extended strong lensing structures of Abell 2744 with the deepest JWST imaging
We present a new parametric lens model for the massive galaxy cluster Abell 2744 based
on new ultra-deep JWST imaging taken in the framework of the UNCOVER program. These …
on new ultra-deep JWST imaging taken in the framework of the UNCOVER program. These …
New high-precision strong lensing modeling of Abell 2744-Preparing for JWST observations
P Bergamini, A Acebron, C Grillo, P Rosati… - Astronomy & …, 2023 - aanda.org
We present a new strong lensing (SL) model of the Hubble Frontier Fields (HFF) galaxy
cluster Abell 2744, at z= 0.3072, by exploiting archival Hubble Space Telescope (HST) …
cluster Abell 2744, at z= 0.3072, by exploiting archival Hubble Space Telescope (HST) …
Inferences on the timeline of reionization at z ∼ 8 from the KMOS Lens-Amplified Spectroscopic Survey
CA Mason, A Fontana, T Treu… - Monthly Notices of …, 2019 - academic.oup.com
Detections and non-detections of Lyman alpha (Lyα) emission from z> 6 galaxies (< 1 Gyr
after the big bang) can be used to measure the timeline of cosmic reionization. Of key …
after the big bang) can be used to measure the timeline of cosmic reionization. Of key …
An excess of small-scale gravitational lenses observed in galaxy clusters
Cold dark matter (CDM) constitutes most of the matter in the Universe. The interplay
between dark and luminous matter in dense cosmic environments, such as galaxy clusters …
between dark and luminous matter in dense cosmic environments, such as galaxy clusters …