Recent observations of GN-z11 with JWST have revealed a Ly$\alpha$ emission
line with an equivalent width of 18$2$ angstroms. At z=10.6, this galaxy is
expected to lie in the heart of reionization. We use a series of inhomogeneous
reionization simulations to derive the distribution of the Ly$\alpha$ EW after
traveling through the neutral intergalactic medium with varying average neutral
gas fraction, $x_HI$. We use these distribution to place an upper limit of
$x_HI < $ 0.88 at z=10.6 at 95% confidence level. We compare our upper limit
to different reionization history models, which include the recently identified
enhancement at the bright end of the luminosity function at z>8. We find that
models in which faint galaxies have higher escape fraction compared to bright
galaxies are favored by the new data.
%0 Generic
%1 bruton2023universe
%A Bruton, Sean
%A Lin, Yu-Heng
%A Scarlata, Claudia
%A Hayes, Matthew J.
%D 2023
%K tifr
%T The Universe is at Most 88% Neutral at z=10.6
%U http://arxiv.org/abs/2303.03419
%X Recent observations of GN-z11 with JWST have revealed a Ly$\alpha$ emission
line with an equivalent width of 18$2$ angstroms. At z=10.6, this galaxy is
expected to lie in the heart of reionization. We use a series of inhomogeneous
reionization simulations to derive the distribution of the Ly$\alpha$ EW after
traveling through the neutral intergalactic medium with varying average neutral
gas fraction, $x_HI$. We use these distribution to place an upper limit of
$x_HI < $ 0.88 at z=10.6 at 95% confidence level. We compare our upper limit
to different reionization history models, which include the recently identified
enhancement at the bright end of the luminosity function at z>8. We find that
models in which faint galaxies have higher escape fraction compared to bright
galaxies are favored by the new data.
@misc{bruton2023universe,
abstract = {Recent observations of GN-z11 with JWST have revealed a Ly$\alpha$ emission
line with an equivalent width of 18$\pm 2$ angstroms. At z=10.6, this galaxy is
expected to lie in the heart of reionization. We use a series of inhomogeneous
reionization simulations to derive the distribution of the Ly$\alpha$ EW after
traveling through the neutral intergalactic medium with varying average neutral
gas fraction, $x_{HI}$. We use these distribution to place an upper limit of
$x_{HI} < $ 0.88 at z=10.6 at 95% confidence level. We compare our upper limit
to different reionization history models, which include the recently identified
enhancement at the bright end of the luminosity function at z>8. We find that
models in which faint galaxies have higher escape fraction compared to bright
galaxies are favored by the new data.},
added-at = {2023-03-08T05:17:59.000+0100},
author = {Bruton, Sean and Lin, Yu-Heng and Scarlata, Claudia and Hayes, Matthew J.},
biburl = {https://www.bibsonomy.org/bibtex/29ceecc5250e421f33745be4ec27650ab/citekhatri},
interhash = {e68c5702a204fdca33028cc1a16ceb32},
intrahash = {9ceecc5250e421f33745be4ec27650ab},
keywords = {tifr},
note = {cite arxiv:2303.03419Comment: 7 pages, 3 figures},
timestamp = {2023-03-08T05:17:59.000+0100},
title = {The Universe is at Most 88% Neutral at z=10.6},
url = {http://arxiv.org/abs/2303.03419},
year = 2023
}