Results 21 to 30 of about 26,307 (200)
HST UV Spectroscopy of the Dwarf Starburst Galaxy Pox 186
Studying the galaxies responsible for reionization is often conducted through local reionization-era analogs; however, many of these local analogs are too massive to be representative of the low-mass star-forming galaxies that are thought to play a ...
Noah S. J. Rogers +6 more
doaj +1 more source
High resolution simulations of the reionization of an isolated Milky Way - M31 galaxy pair [PDF]
We present the results of a set of numerical simulations aimed at studying reionization at galactic scale. We use a high resolution simulation of the formation of the Milky Way-M31 system to simulate the reionization of the local group.
Aubert, D. +7 more
core +2 more sources
Impact of general reionization scenarios on extraction of inflationary parameters [PDF]
Determination of whether the Harrison--Zel'dovich spectrum for primordial scalar perturbations is consistent with observations is sensitive to assumptions about the reionization scenario.
Alessandro Melchiorri +9 more
core +4 more sources
Detecting Helium Reionization with Fast Radio Bursts
Fast radio bursts (FRB) probe the electron density of the universe along the path of propagation, making high redshift FRB sensitive to the helium reionization epoch.
Linder, Eric V.
core +1 more source
Reionization and Beyond: detecting the peaks of the cosmological 21cm signal [PDF]
[ABRIDGED] The cosmological 21cm signal is set to become the most powerful probe of the early Universe, with first generation interferometers aiming to make statistical detections of reionization. There is increasing interest also in the pre-reionization
Ewall-Wice, Aaron +2 more
core +1 more source
We report the most sensitive upper limits to date on the 21 cm epoch of reionization power spectrum using 94 nights of observing with Phase I of the Hydrogen Epoch of Reionization Array (HERA).
The HERA Collaboration: Zara Abdurashidova +93 more
doaj +1 more source
The Universe is at Most 88% Neutral at z = 10.6
Recent observations of GN-z11 with JWST have revealed a Ly α emission line with an equivalent width (EW) of 18 ± 2 Å. At z = 10.6, this galaxy is expected to lie in the heart of reionization.
Sean Bruton +3 more
doaj +1 more source
Simulating Reionization: Character and Observability [PDF]
In recent years there has been considerable progress in our understanding of the nature and properties of the reionization process. In particular, the numerical simulations of this epoch have made a qualitative leap forward, reaching sufficiently large ...
Bond, J. Richard +5 more
core +1 more source
Cosmic reionization constraints on the nature of cosmological perturbations [PDF]
We study the reionization history of the Universe in cosmological models with non-Gaussian density fluctuations, taking them to have a renormalized $\chi^2$ probability distribution function parametrized by the number of degrees of freedom, $\nu$.
Avelino, Pedro P, Liddle, Andrew R
core +2 more sources
Reionization Histories of Milky Way Mass Halos
We investigate the connection between the epoch of reionization and the present day universe, by examining the extended mass reionization histories of dark matter halos identified at z=0.
Abel, Tom +3 more
core +2 more sources

