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The evolution of the intergalactic medium
The bulk of cosmic matter resides in a dilute reservoir that fills the space between galaxies,
the intergalactic medium (IGM). The history of this reservoir is intimately tied to the cosmic …
the intergalactic medium (IGM). The history of this reservoir is intimately tied to the cosmic …
Galaxies in the first billion years after the big bang
DP Stark - Annual Review of Astronomy and Astrophysics, 2016 - annualreviews.org
In the past five years, deep imaging campaigns conducted with the Hubble Space
Telescope (HST) and ground-based observatories have delivered large samples of galaxies …
Telescope (HST) and ground-based observatories have delivered large samples of galaxies …
Metal-poor star formation at z > 6 with JWST: new insight into hard radiation fields and nitrogen enrichment on 20 pc scales
MW Top**, DP Stark, P Senchyna… - Monthly Notices of …, 2024 - academic.oup.com
Nearly a decade ago, we began to see indications that reionization-era galaxies power hard
radiation fields rarely seen at lower redshift. Most striking were detections of nebular C iv …
radiation fields rarely seen at lower redshift. Most striking were detections of nebular C iv …
EIGER. I. A large sample of [O iii]-emitting galaxies at 5.3< z< 6.9 and direct evidence for local reionization by galaxies
EIGER. I. A Large Sample of [O iii]-emitting Galaxies at 5.3 < z < 6.9 and Direct Evidence for
Local Reionization by Galaxies - IOPscience Skip to content IOP Science home Accessibility …
Local Reionization by Galaxies - IOPscience Skip to content IOP Science home Accessibility …
Reionization era bright emission line survey: selection and characterization of luminous interstellar medium reservoirs in the z> 6.5 universe
RJ Bouwens, R Smit, S Schouws… - The Astrophysical …, 2022 - iopscience.iop.org
Abstract The Reionization Era Bright Emission Line Survey (REBELS) is a cycle-7 ALMA
Large Program (LP) that is identifying and performing a first characterization of many of the …
Large Program (LP) that is identifying and performing a first characterization of many of the …
Lyα Emission at z= 7–13: Clear Evolution of Lyα Equivalent Width Indicating a Late Cosmic Reionization History
We present the evolution of Lyα emission derived from 53 galaxies at z= 6.6–13.2, which
have been identified by multiple JWST/NIRSpec spectroscopy programs of Early Release …
have been identified by multiple JWST/NIRSpec spectroscopy programs of Early Release …
First results from hera phase i: Upper limits on the epoch of reionization 21 cm power spectrum
We report upper limits on the Epoch of Reionization 21 cm power spectrum at redshifts 7.9
and 10.4 with 18 nights of data (∼ 36 hr of integration) from Phase I of the Hydrogen Epoch …
and 10.4 with 18 nights of data (∼ 36 hr of integration) from Phase I of the Hydrogen Epoch …
Peering into cosmic reionization: Lyα visibility evolution from galaxies at z= 4.5–8.5 with JWST
The resonant scattering interaction between Lyα photons and neutral hydrogen implies that
a partially neutral intergalactic medium has the ability to significantly impact the detectability …
a partially neutral intergalactic medium has the ability to significantly impact the detectability …
A remarkably luminous galaxy at z= 11.1 measured with Hubble Space Telescope grism spectroscopy
PA Oesch, G Brammer, PG Van Dokkum… - The Astrophysical …, 2016 - iopscience.iop.org
ABSTRACT We present Hubble WFC3/IR slitless grism spectra of a remarkably bright z≳ 10
galaxy candidate, GN-z11, identified initially from CANDELS/GOODS-N imaging data. A …
galaxy candidate, GN-z11, identified initially from CANDELS/GOODS-N imaging data. A …
JADES: The emergence and evolution of Lyα emission and constraints on the intergalactic medium neutral fraction
The rest-frame UV recombination emission line Lyα can be powered by ionising photons
from young massive stars in star-forming galaxies, but the fact that it can be resonantly …
from young massive stars in star-forming galaxies, but the fact that it can be resonantly …