Double-peaked Lyα profiles during reionization require sightlines through nearby voids a few cMpc from the galaxy and a sufficiently strong local ionizing background, with occurrence probability rising sharply with background intensity.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
Varying the star formation history of galaxies while keeping total ionizing photons fixed changes the size and warmth of ionized regions, altering the topology of reionization and the 21-cm global signal and power spectrum.
citing papers explorer
-
Double-Peaked Ly$\alpha$ Emission during Reionization Requires Nearby Voids and a Favorable Local Ionizing Background
Double-peaked Lyα profiles during reionization require sightlines through nearby voids a few cMpc from the galaxy and a sufficiently strong local ionizing background, with occurrence probability rising sharply with background intensity.
-
POLAR-II: modeling star formation history of galaxies on the 21-cm signal from Epoch of Reionization
Varying the star formation history of galaxies while keeping total ionizing photons fixed changes the size and warmth of ionized regions, altering the topology of reionization and the 21-cm global signal and power spectrum.