The Effects of Population III X-ray and Radio Backgrounds on the Cosmological 21-cm Signal

Oct. 22, 2019

Richard H. Mebane, Jordan Mirocha, Steven R. Furlanetto

Results from EDGES High-Band: III. New Constraints on Parameters of the Early Universe

Jan. 30, 2019

Raul A. Monsalve, Anastasia Fialkov, Judd D. Bowman, Alan E. E. Rogers, Thomas J. Mozdzen, Aviad Cohen, Rennan Barkana, Nivedita Mahesh

A Ground Plane Artifact that Induces an Absorption Profile in Averaged Spectra from Global 21-cm Measurements - with Possible Application to EDGES

Oct. 21, 2018

Richard F. Bradley, Keith Tauscher, David Rapetti, Jack O. Burns

A new goodness-of-fit statistic and its application to 21-cm cosmology

Sept. 28, 2018

Keith Tauscher, David Rapetti, Jack O. Burns

Results from EDGES High-Band: II. Constraints on Parameters of Early Galaxies

June 20, 2018

R. Monsalve, B. Greig, J. Bowman, A. Mesinger, A. Rogers, T. Mozdzen, N. Kern, N. Mahesh

Science on the lunar surface facilitated by low latency telerobotics from a Lunar Orbital Platform - Gateway

April 21, 2018

Jack O. Burns, Benjamin Mellinkoff, Matthew Spydell, Terrence Fong, David A. Kring, William D. Pratt, Timothy Cichan, Christine M. Edwards

The American Space Exploration Narrative from the Cold War through the Obama Administration

March 29, 2018

Dora Holland, Jack O. Burns

What Does the First Highly-redshifted 21-cm Detection Tell us about Early Galaxies?

March 8, 2018

Jordan Mirocha, Steven R. Furlanetto

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An Absorption Profile Centered at 78 megahertz in the Sky-averaged Spectrum

March 1, 2018

From Nature: After stars formed in the early Universe, their ultraviolet light is expected, eventually, to have penetrated the primordial hydrogen gas and altered the excitation state of its 21-centimetre hyperfine line. This alteration would cause the gas to absorb photons from the cosmic microwave background, producing a spectral distortion...

Global 21cm Signal Extraction from Foreground and Instrumental Effects I: Pattern Recognition Framework for Separation using Training Sets

Nov. 8, 2017

Keith Tauscher, David Rapetti, Jack O. Burns, Eric R. Switzer

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