Results 121 to 130 of about 8,595 (212)
Context. Galaxies may suffer some starburst and quenched periods in their history due to galaxy mergers and feedback. However, semi-numerical simulations of the Epoch of Reionization (EoR) do not accurately model the effects of the star formation history
Ma Qing-Bo +8 more
doaj +1 more source
Reionization Parameter Inference from 3D Minkowski Functionals of the 21 cm Signals
The Minkowski functionals (MFs), a set of topological summary statistics, have emerged as a powerful tool for extracting non-Gaussian information.
Kangning Diao +3 more
doaj +1 more source
The SPHINX public data release
Context. Low-ionisation state (LIS) metal absorption lines, such as Si II λ1526, are widely used to trace the properties and dynamics of the interstellar medium (ISM) in galaxies.
Mauerhofer Valentin +13 more
doaj +1 more source
Peering into the dark (ages) with low-frequency space interferometers: Using the 21-cm signal of neutral hydrogen from the infant universe to probe fundamental (Astro)physics. [PDF]
Koopmans LVE +29 more
europepmc +1 more source
We analyse the impact of the decaying magnetic turbulence of primordial magnetic fields (PMFs) and ambipolar diffusion on the ionisation and thermal history of the Dark Ages Universe (30 ≤ z ≤ 300), and its imprint on the spectral profile of the global ...
Novosyadlyj B. +3 more
doaj +1 more source
Fluctuations in 21-cm emission after reionization
The fluctuations in the emission of redshifted 21-cm photons from neutral intergalactic hydrogen will provide an unprecedented probe of the reionization era.
Loeb, Abraham, Wyithe, J. Stuart B.
core +1 more source
Generative models of 21 cm Epoch of Reionisation lightcones with 3D scattering transforms
The 21 cm signal from the Epoch of Reionisation (EoR) is observed as a 3D dataset known as a lightcone, consisting of two spatial sky plane axes and a redshift (frequency) axis.
Hothi Ian +3 more
doaj +1 more source
We used the ultra-deep GLIMPSE JWST/NIRCam survey to constrain the faint end of the [O III]+Hβ luminosity function (LF) down to 1039erg s−1 at z ∼ 7 − 9 behind the lensed Hubble Frontier Field galaxy cluster Abell S1063.
Korber Damien +14 more
doaj +1 more source
Extremely ultraviolet-bright starbursts at the end of cosmic reionization
We present a study of 27 very UV-bright (−22.0 ≲ MUV ≲ −24.4) star-forming galaxies at z ∼ 6 identified in the Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) survey.
Marques-Chaves R. +24 more
doaj +1 more source

