activity
20152024
most citedHydrogen Epoch of Reionization Array (HERA)

657 citations · 3.7k across the 74 of their papers we have counts for

collaborators
Showing 2017Show all

7 papers · 1 filter

astro-ph.IM2017★ 45 cited

Polarized Redundant-Baseline Calibration for 21 cm Cosmology Without Adding Spectral Structure

Joshua S. Dillon, Saul A. Kohn, Aaron R. Parsons +8

21 cm cosmology is a promising new probe of the evolution of visible matter in our universe, especially during the poorly-constrained Cosmic Dawn and Epoch of Reionization. However…

hep-ex2017★ 21 cited

Cosmogenic neutron production at Daya Bay

Daya Bay Collaboration, F. P. An, A. B. Balantekin +197

Neutrons produced by cosmic ray muons are an important background for underground experiments studying neutrino oscillations, neutrinoless double beta decay, dark matter, and other…

astro-ph.CO2017★ 8 cited

Galactic wind X-ray heating of the intergalactic medium during the Epoch of Reionization

Avery Meiksin, Sadegh Khochfar, Jan-Pieter Paardekooper +2

The diffuse soft X-ray emissivity from galactic winds is computed during the Epoch of Reionization (EoR). We consider two analytic models, a pressure-driven wind and a superbubble…

physics.ins-det2017★ 14 cited

Seasonal Variation of the Underground Cosmic Muon Flux Observed at Daya Bay

F. P. An, A. B. Balantekin, H. R. Band +199

The Daya Bay Experiment consists of eight identically designed detectors located in three underground experimental halls named as EH1, EH2, EH3, with 250, 265 and 860 meters of wat…

physics.ins-det2017

The Single-Phase ProtoDUNE Technical Design Report

B. Abi, R. Acciarri, M. A. Acero +824

ProtoDUNE-SP is the single-phase DUNE Far Detector prototype that is under construction and will be operated at the CERN Neutrino Platform (NP) starting in 2018. ProtoDUNE-SP, a cr…

astro-ph.CO2017★ 30 cited

Constraining Polarized Foregrounds for EOR Experiments II: Polarization Leakage Simulations in the Avoidance Scheme

C. D. Nunhokee, G. Bernardi, S. A. Kohn +7

A critical challenge in the observation of the redshifted 21-cm line is its separation from bright Galactic and extragalactic foregrounds. In particular, the instrumental leakage o…