most citedA new MWA limit on the 21 cm Power Spectrum at Redshifts 13 17

67 citations · 76 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.CO20212 cited

Epoch of Reionization Power Spectrum Limits from Murchison Widefield Array Data Targeted at EoR1 Field

M. Rahimi, B. Pindor, J. L. B. Line +28

Current attempts to measure the 21cm Power Spectrum of neutral hydrogen during the Epoch of Reionization are limited by systematics which produce measured upper limits above both t…

astro-ph.CO20217 cited

Constraining the 21cm brightness temperature of the IGM at =6.6 around LAEs with the Murchison Widefield Array

Cathryn M. Trott, C. H. Jordan, J. L. B. Line +29

The locations of Ly- emitting galaxies (LAEs) at the end of the Epoch of Reionisation (EoR) are expected to correlate with regions of ionised hydrogen, traced by the redshifted…

astro-ph.SR2021

The Rise and Fall of the Eclipsing Binary HS Hydrae

James R. A. Davenport, Diana Windemuth, Karen Warmbein +3

HS Hydrae is a short period eclipsing binary (P_orb=1.57 day) that belongs to a rare group of systems observed to have rapidly changing inclinations. This evolution is due to a thi…

astro-ph.CO202167 cited

A new MWA limit on the 21 cm Power Spectrum at Redshifts 13 17

S. Yoshiura, B. Pindor, J. L. B. Line +29

Observations in the lowest MWA band between MHz have the potential to constrain the distribution of neutral hydrogen in the intergalactic medium at redshift .…

astro-ph.HE2020

Neutron Star Extreme Matter Observatory: A kilohertz-band gravitational-wave detector in the global network

K. Ackley, V. B. Adya, P. Agrawal +160

Gravitational waves from coalescing neutron stars encode information about nuclear matter at extreme densities, inaccessible by laboratory experiments. The late inspiral is influen…

astro-ph.SR2020

APOGEE Net: Improving the derived spectral parameters for young stars through deep learning

Richard Olney, Marina Kounkel, Chad Schillinger +6

Machine learning allows efficient extraction of physical properties from stellar spectra that have been obtained by large surveys. The viability of ML approaches has been demonstra…