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Quantifying EoR delay spectrum contamination from diffuse radio emission
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Optimizing sparse RFI prediction using deep learning
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H I 21‐cm Cosmology and the Bispectrum: Closure Diagnostics in Massively Redundant Interferometric Arrays;
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Detecting Cosmic Reionization Using the Bispectrum Phase;
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Polarized redundant-baseline calibration for 21-cm cosmology without adding spectral structure;
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The hydrogen epoch of reionization array dish III: measuring chromaticity of prototype element with reflectometry;
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Sensitivity of the Hydrogen Epoch of Reionization Array and its Build-out Stages to One-point Statistics from Redshifted 21 cm Observations;
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Redundant interferometric calibration as a complex optimization problem;
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Polarized Foreground Power Spectra from the HERA-19 Commissioning Array;
Kohn, Saul; et al. arxiv; February 2018
Unlocking sensitivity for visibility-based estimators of the 21 cm reionization power spectrum;
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Foreground and sensitivity analysis for broadband (2D) 21 cm-Lya and 21 cm-Ha correlation experiments probing the epoch of reionization;
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Constraining polarized foregrounds for EoR experiments II: Polarization leakage simulations in the avoidance scheme;
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Emulating simulations of cosmic dawn for 21cm power spectrum constraints on cosmology, reionization, and x-ray heating;
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An Efficient Feedback Calibration Algorithm for Direct Imaging Radio Telescopes;
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The impact of modeling errors on interferometer calibration for 21 cm power spectra;
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pyuvdata: an interface for astronomical interferometric datasets in python;
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Limits on polarized leakage for the PAPER Epoch of Reionization measurements at 126 and 164 MHz;
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First demonstration of ECHO: An external calibrator for hydrogen observatories;
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A Generic and Efficient E-field Parallel Imaging Correlator for Next-Generation Radio Telescopes;
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Spherical harmonic analyses of intensity mapping power spectra;
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First season MWA power spectrum results at redshift 7;
Beardsley, A.P.; et al. arxiv; APJ; 9 December, 2016
Brute-force mapmaking with compact interferometers: a MITEoR northern sky map from 128 to 175 MHz;
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The Hydrogen Epoch of Reionization Array dish II: Characterization of spectral structure with electromagnetic simulations and its science implications;
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An improved model of diffuse galactic radio emission from 10 MHz to 5 THz;
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Upper limits on the 21 cm power spectrum at z=5.9 from quasar absorption line spectroscopy;
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Redundant array configurations for 21 cm cosmology;
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The Hydrogen Epoch of Reionization Array dish I: Beam pattern measurements and science implications;
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Contamination of the Epoch of Reionization power spectrum in the presence of foregrounds;
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The Murchison Widefield Array 21 cm power spectrum analysis methodology;
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A high reliability survey of discrete Epoch of Reionization foreground sources in the MWA EoRo field;
Carroll, P.A.; et al. MNRAS; 8 July, 2016
Effects of antenna beam chromaticity on redshifted 21-cm power spectrum and implications for Hydrogen Epoch of Reionization Array;
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Calibration requirements for detecting the 21 cm epoch of reionization power spectrum and implications for the SKA;
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Constraining polarized foregrounds for EoR experiments I: 2D power spectra from the PAPER-32 imaging array;
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First limits on the 21-cm power spectrum during the Epoch of X-ray heating;
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Optimized beam sculpting with generalized fringe-rate filters;
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Beam-forming errors in Murchison Widefield Array phased array antennas and their effects on Epoch of Reionization science;
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Constraining high-redshift x-ray sources with next generation 21-cm power spectrum measurements;
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The importance of wide-field foreground removal for 21-cm cosmology: a demonstration with early MWA epoch of reionization observations;
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Eliminating the optical depth nuisance from the CMB with 21 cm cosmology;
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Constraining cosmology and ionization history with combined 21 cm power spectrum and global signal measurements;
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PAPER-64 constraints on reionization II: the temperature of the z=8.4 intergalactic medium;
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PAPER-64 constraints on reionization: the 21 cm power spectrum at z=8.4;
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Confirmation of wide-field signatures in redshifted 21 cm power spectra;
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Empirical covariance modeling for 21cm power spectrum estimation: A method demonstration and new limits from early Murchison Widefield Array 128-tile data;
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Measuring phased-array antenna beampatterns with high dynamic range for the Murchison Widefield Array using 137 MHz ORBCOMM satellites;
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Adding context to James Webb Space Telescope surveys with current and future 21cm radio observations;
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The impact of foregrounds on redshift space distortion measurements with the highly redshifted 21-cm line;
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MITEoR: a scalable interferometer for precision 21cm cosmology;
Zheng, H.; et al. MNRAS; 7 October, 2014
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