activity
20092019
most citedBubble size statistics during reionization from 21-cm tomography

75 citations · 160 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA20194 cited

Clues to the nature of dark matter from first galaxies

Boyan K. Stoychev, Keri L. Dixon, Andrea V. Macciò +2

We use thirty-eight high-resolution simulations of galaxy formation between redshift 10 and 5 to study the impact of a 3 keV warm dark matter (WDM) candidate on the high-redshift U…

astro-ph.GA201715 cited

Using Artificial Neural Networks to Constrain the Halo Baryon Fraction during Reionization

David Sullivan, Ilian T. Iliev, Keri L. Dixon

Radiative feedback from stars and galaxies has been proposed as a potential solution to many of the tensions with simplistic galaxy formation models based on CDM, such as the fa…

astro-ph.CO201775 cited

Bubble size statistics during reionization from 21-cm tomography

Sambit K. Giri, Garrelt Mellema, Keri L. Dixon +1

The upcoming SKA1-Low radio interferometer will be sensitive enough to produce tomographic imaging data of the redshifted 21-cm signal from the Epoch of Reionization. Due to the no…

astro-ph.CO201728 cited

A self-consistent 3D model of fluctuations in the helium-ionizing background

Frederick B. Davies, Steven R. Furlanetto, Keri L. Dixon

Large variations in the effective optical depth of the He II Ly forest have been observed at , but the physical nature of these variations is uncertain: either the…

astro-ph.CO200938 cited

The evolution of the helium-ionizing background at z ~ 2-3

Keri L. Dixon, Steven R. Furlanetto

Recent observations suggest that helium became fully ionized around redshift z ~ 3. The HeII optical depth derived from the Lyman-alpha forest decreases substantially from this per…