LyC escape from sphinx galaxies in the Epoch of Reionization
We measure escape fractions, f esc, of ionizing radiation from galaxies in the sphinx suite of
cosmological radiation-hydrodynamical simulations of reionization, resolving haloes with …
cosmological radiation-hydrodynamical simulations of reionization, resolving haloes with …
Rapid reionization by the oligarchs: the case for massive, UV-bright, star-forming galaxies with high escape fractions
The protagonists of the last great phase transition of the universe—cosmic reionization—
remain elusive. Faint star-forming galaxies are leading candidates because they are found …
remain elusive. Faint star-forming galaxies are leading candidates because they are found …
The synchrony of production and escape: half the bright Lyα emitters at z ≈ 2 have Lyman continuum escape fractions ≈50
The ionizing photon escape fraction [Lyman continuum (LyC) f esc] of star-forming galaxies
is the single greatest unknown in the reionization budget. Stochastic sightline effects prohibit …
is the single greatest unknown in the reionization budget. Stochastic sightline effects prohibit …
The universe is reionizing at z∼ 7: bayesian inference of the IGM neutral fraction using Lyα emission from galaxies
CA Mason, T Treu, M Dijkstra, A Mesinger… - The Astrophysical …, 2018 - iopscience.iop.org
We present a new flexible Bayesian framework for directly inferring the fraction of neutral
hydrogen in the intergalactic medium (IGM) during the Epoch of Reionization (EoR, z∼ 6 …
hydrogen in the intergalactic medium (IGM) during the Epoch of Reionization (EoR, z∼ 6 …
The Keck Lyman Continuum Spectroscopic Survey (KLCS): The Emergent Ionizing Spectrum of Galaxies at z∼ 3∗
The Keck Lyman Continuum Spectroscopic Survey (KLCS): The Emergent Ionizing Spectrum
of Galaxies at z ∼ 3 - IOPscience This site uses cookies. By continuing to use this site you …
of Galaxies at z ∼ 3 - IOPscience This site uses cookies. By continuing to use this site you …
The CANDELS/SHARDS multiwavelength catalog in GOODS-N: photometry, photometric redshifts, stellar masses, emission-line fluxes, and star formation rates
G Barro, PG Pérez-González, A Cava… - The Astrophysical …, 2019 - iopscience.iop.org
We present a WFC3 F160W (H-band) selected catalog in the CANDELS/GOODS-N field
containing photometry from the ultraviolet (UV) to the far-infrared (IR), photometric redshifts …
containing photometry from the ultraviolet (UV) to the far-infrared (IR), photometric redshifts …
The THESEUS space mission concept: science case, design and expected performances
THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for
investigating the early Universe and at providing a substantial advancement of multi …
investigating the early Universe and at providing a substantial advancement of multi …
Modeling the radio background from the first black holes at cosmic dawn: implications for the 21 cm absorption amplitude
A Ewall-Wice, TC Chang, J Lazio, O Doré… - The Astrophysical …, 2018 - iopscience.iop.org
We estimate the 21 cm radio background from accretion onto the first intermediate-mass
black holes between z≈ 30 and z≈ 16. Combining potentially optimistic, but plausible …
black holes between z≈ 30 and z≈ 16. Combining potentially optimistic, but plausible …
Searching for Islands of Reionization: A Potential Ionized Bubble Powered by a Spectroscopic Overdensity at z= 8.7
RL Larson, SL Finkelstein, TA Hutchison… - The Astrophysical …, 2022 - iopscience.iop.org
We present the results from a spectroscopic survey using the MOSFIRE near-infrared
spectrograph on the 10 m Keck telescope to search for Lyα emission from candidate …
spectrograph on the 10 m Keck telescope to search for Lyα emission from candidate …
(Re)Solving reionization with Lyα: how bright Lyα Emitters account for the z ≈ 2–8 cosmic ionizing background
The cosmic ionizing emissivity from star-forming galaxies has long been anchored to UV
luminosity functions. Here, we introduce an emissivity framework based on Lyα emitters …
luminosity functions. Here, we introduce an emissivity framework based on Lyα emitters …