Results 101 to 110 of about 8,595 (212)
We present very deep (≈11 hours on-source) JWST/MIRI low-resolution spectroscopy of the rest-frame optical emission of U37126, a UV-bright (MUV ≃ −20) mildly lensed (μ ≃ 2.2) galaxy at z = 10.255.
Marques-Chaves R. +33 more
doaj +1 more source
Weighing gas-rich starless halos: Dark matter parameter inference based on gas distributions
Context. Reionization-limited H I clouds (RELHICs) are starless dark matter halos that retain a significant neutral hydrogen (H I) reservoir. The gas resides in near hydrostatic equilibrium within the dark matter potential and in thermal equilibrium with
Turini Francesco +1 more
doaj +1 more source
Reionization of the inhomogeneous universe
A model of the density distribution in the intergalactic medium, motivated by that found in numerical simulations, is used to demonstrate the effect of a clumpy IGM and discrete sources on the reionization of the universe.
Rees, M.J. (Cambridge Univ. (United Kingdom). Inst. of Astronomy) +6 more
core
High-redshift Quasars as Probes of Cosmic Reionization
Cosmic reionization was the last major phase transition of atomic hydrogen in the IGM, empowered by the first luminous sources in the universe. With extensive studies over the past two decades, the timeline of the second half of reionization has been ...
Jin, Xiangyu
core +3 more sources
Discriminating Planck reionisation histories with the kSZ effect
The epoch of reionisation is a key phase in cosmic history, but its detailed evolution remains poorly constrained by current cosmic microwave background (CMB) observations.
Douspis M. +7 more
doaj +1 more source
10 pages, LaTeX, to appear in the proceedings of "Galaxy Evolution: Theory and Observations", Cozumel, Mexico, April 2002. Eds. V. Avila-Reese, C. Firmani, C. Frenk, & C. Allen, RevMexAA SC (2002)
openaire +2 more sources
Neutral beam system reionization losses [PDF]
A slow, linear pressure rise in the drift ducts of the PLT neutral beam systems, and the resulting reionization losses of neutral beam power, are reported and examined.
Stewart, L. D., L.D. Stewart
core +1 more source
Studying dark gaps in Lyman-α forest transmission with large reionization simulations
The physical conditions of the intergalactic medium (IGM) during the final stages of cosmic reionization (z ∼ 5.0 − 6.0) are not yet fully understood.
Maity Barun +3 more
doaj +1 more source
Joining Bits and Pieces of Reionization History [PDF]
International audienceCosmic microwave background (CMB) temperature and polarization anisotropies from Planck have estimated a lower value of the optical depth to reionization (τ) compared to WMAP.
George F. Smoot +7 more
core +1 more source
Reionization and structure formation with ARCADE [PDF]
To be published in the proceedings of "The Cosmic Microwave Background and its Polarization", New Astronomy Reviews, (eds. S. Hanany and K.A. Olive)
openaire +2 more sources

