Results 1 to 10 of about 8,595 (212)
The Impact of Patchy Reionization on Ultrafaint Dwarf Galaxies [PDF]
We investigate how patchy reionization affects the star formation history (SFH) and stellar metallicity of ultrafaint dwarf galaxies (UFDs). Patchy reionization refers to varying ultraviolet background strengths depending on a galaxy’s environment ...
Jaeeun Kim +5 more
doaj +3 more sources
Cosmic Reionization on Computers: Properties of the Post-reionization IGM [PDF]
Abstract We present a comparison between several observational tests of the post-reionization intergalactic medium and the numerical simulations of reionization completed under the Cosmic Reionization On Computers (CROC) project. The CROC simulations match the gap distribution reasonably well, and also provide a good match for the ...
Gnedin, Nickolay Y. +2 more
openaire +3 more sources
Reaction Environment Engineering for Selective C3+ Formation in CO2 Electroreduction: Progress and Perspectives [PDF]
This work focuses on how to improve the selectivity and activity of electrocatalytic CO2 reduction to C3+ products, by the integration of electrocatalyst and electrolyte co‐design. We summarize key C3+ formation mechanisms and provide a comprehensive reaction network through thermodynamic analysis.
Ling Chen, Damien Voiry, Yan Jiao
wiley +3 more sources
A SPectroscopic Survey of Biased Halos In the Reionization Era (ASPIRE): JWST Supports Earlier Reionization around [O iii] Emitters [PDF]
Understanding when and how reionization happened is crucial for studying the early structure formation and the properties of the first galaxies in the Universe. At z > 5.5, the observed intergalactic medium (IGM) optical depth shows a significant scatter,
Xiangyu Jin +24 more
doaj +3 more sources
The epoch of reionization [PDF]
We have modelled the process of reionization of the IGM by photoionization by galaxies, in order to predict the epoch of reionization. We use a sophisticated semi-analytic model to track the formation of galaxies. Our study represents a much more complete and physically consistent modelling of reionization than has been conducted in the past ...
Benson, A.J. +3 more
openaire +3 more sources
The reionization of carbon [PDF]
Observations suggest that CII was more abundant than CIV in the intergalactic medium towards the end of the hydrogen reionization epoch. This transition provides a unique opportunity to study the enrichment history of intergalactic gas and the growth of the ionizing background (UVB) at early times.
Finlator, Kristian +5 more
openaire +3 more sources
CEMPlifying reionization [PDF]
14 pages, 13 figures, Accepted in MNRAS, Comments ...
Mahavir Sharma, Tom Theuns, Carlos Frenk
openaire +3 more sources
AbstractThe transformation of cold neutral intergalactic hydrogen into a highly ionized warm plasma marks the end of the cosmic dark ages and the beginning of the age of galaxies. The details of this process reflect the nature of the early sources of radiation and heat, the statistical characteristics of the large-scale structure of the Universe, the ...
Nickolay Y. Gnedin, Piero Madau
openaire +2 more sources
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 ...
J Richard Bond (16065854) +5 more
core +2 more sources
The epoch of helium reionization [PDF]
39 pages, including 13 figures, submitted to ...
Sokasian, A., Abel, T., Hernquist, L.
openaire +4 more sources

