Steven R. Furlanetto

TL;DR: In this article, the authors demonstrate that observations of the galaxy populations in the vicinity of the deepest troughs can distinguish two competing models for these features: deep voids where the ionizing background is weak due to fluctuations in the mean free path of ionizing photons would show a deficit of galaxies, while residual temperature variations from extended, inhomogeneous reionization would show an overdensity of galaxies.

TL;DR: In this paper , a Bayesian jackknife test for assessing the probability that a data set contains biased subsets, and, if so, which of the subsets are likely to be biased.

TL;DR: The cosmic dark ages are the mysterious epoch during which the pristine gas began to condense and ultimately form the first stars as mentioned in this paper, and it is only recently that technology has allowed the beginnings of observational insight into this epoch.

TL;DR: The cosmic dark ages are the mysterious epoch during which the pristine gas began to condense and ultimately form the first stars as discussed by the authors, and it is only recently that technology has allowed the beginnings of observational insight into this epoch.

TL;DR: It is shown that in the future, as the noise level of the data comes down, CLEAN and DPSS are most capable of reproducing the frequency structure in the visibilities of HERA data, and that techniques that incorporate high wavenumbers in delay space in their modeling are best suited for inpainting over narrowband RFI.