Results 101 to 110 of about 31,186 (206)
How galaxies drive reionization and what governs its geometry remain fundamental questions. We present JWST/NIRCam wide-field slitless spectroscopy (WFSS) observations toward two of the most Ly α -transmissive QSO sight lines near the end of reionization.
Yongda Zhu +8 more
doaj +1 more source
Neutrino communication, intergalactic transit, and Astrobiology. [PDF]
Shapshak P.
europepmc +1 more source
The 2023 Flight of the Faint Intergalactic-medium Redshifted Emission Balloon
The second iteration of the Faint Intergalactic-medium Redshifted Emission Balloon (FIREBall-2) is a UV multiobject spectrograph designed to detect emission from the circumgalactic and circumquasar medium at low redshifts ( z < 1).
Drew M. Miles +36 more
doaj +1 more source
Lyman limit systems (LLSs) are dense hydrogen clouds with high enough H i column densities to absorb Lyman continuum photons emitted from distant quasars.
Jiawen Fan +3 more
doaj +1 more source
Neutrino and EM asterometric detection of habitable exoplanets. [PDF]
Shapshak P.
europepmc +1 more source
Quasar Radiative Feedback May Suppress Galaxy Growth on Intergalactic Scales at z = 6.3
We present observational evidence that intense ionizing radiation from a luminous quasar suppresses nebular emission in nearby galaxies on intergalactic scales at z = 6.3.
Yongda Zhu +29 more
doaj +1 more source
The Quasar Proximity Effect as an Alternative Probe of Quasar Pair Distances
Recently discovered quasar pairs at high redshifts ( z ≳ 5) are likely precursors to supermassive black hole mergers, providing a promising window to high-redshift quasar growth mechanisms.
Huanqing Chen +2 more
doaj +1 more source
Cosmic-void observations reconciled with primordial magnetogenesis. [PDF]
Hosking DN, Schekochihin AA.
europepmc +1 more source
As part of the HIERACHY program, we collect the high signal-to-noise ratio and high-spectral resolution optical spectra of 25 quasars at z ≈ 4–5 to constrain the C iv evolution at z ≈ 3–5.
Xiaodi Yu +5 more
doaj +1 more source

