REVIEW 3 cited by
A new parameterization of the reionisation history
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
read the original abstract
Motivated by the current constraints on the epoch of reionisation from recent cosmic microwave background observations, ionising background measurements of star-forming galaxies, and low redshifts line-of-sight probes, we propose a new data-motivated parameterisation of the history of the average ionisation fraction. This parameterisation describes a flexible redshift-asymmetric reionisation process in two regimes that is capable of fitting all the current constraints.
Forward citations
Cited by 3 Pith papers
-
CAMB v2: cosmological power spectra for high-precision surveys
CAMB v2's default settings produce lensed CMB and matter power spectra converged to 10^-3 over survey-relevant scales, using a new flat-Bessel mapping for hyperspherical Bessel functions.
-
No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization
Epoch-of-reionization hydrogen probes, combined with CMB and BAO data but no CMB polarization, yield tau_reio = 0.067 +/- 0.011 and leave the dynamical-dark-energy preference at ~2 sigma.
-
Intensity fluctuations of radio halo in galaxy cluster: Insights from power spectrum estimation
Angular power spectra of 610 MHz radio halos show excess power-law fluctuations only in Abell 2744, requiring multiplicative C_ℓ ∝ ℓ^{-3} structure atop an exponential profile and consistent with ICM turbulence.
Discussion (0). Continue with ORCID to comment.