Showing 1–20 of 62 results
/ Date/ Name
Jul 15, 2019A Roadmap for Astrophysics and Cosmology with High-Redshift 21 cm Intensity MappingOct 8, 2012The Baryon Acoustic Oscillation Broadband and Broad-beam Array: Design Overview and Sensitivity ForecastsJul 29, 2013A Flux Scale for Southern Hemisphere 21cm EoR ExperimentsNov 17, 2023Direct Optimal Mapping Image Power Spectrum and its Window FunctionsSep 12, 2024A Radio Technosignature Search of TRAPPIST-1 with the Allen Telescope ArrayFeb 13, 2024A demonstration of the effect of fringe-rate filtering in the Hydrogen Epoch of Reionization Array delay power spectrum pipelineMar 23, 2023Precise Measurements of Self-absorbed Rising Reverse Shock Emission from Gamma-ray Burst 221009ANov 4, 2025Exploring One-point Statistics in HERA Phase I Data: Effects of Foregrounds and Systematics on Measuring One-Point StatisticsNov 15, 2024Impacts and Statistical Mitigation of Missing Data on the 21cm Power Spectrum: A Case Study with the Hydrogen Epoch of Reionization ArrayApr 19, 2021Validation of the HERA Phase I Epoch of Reionization 21 cm Power Spectrum Software PipelineSep 4, 2019A simplified, lossless re-analysis of PAPER-64Feb 7, 2018The HERA-19 Commissioning Array: Direction Dependent EffectsJan 12, 2017The Hydrogen Epoch of Reionization Array Dish III: Measuring Chromaticity of Prototype Element with ReflectometryFeb 20, 2015PAPER-64 Constraints on Reionization: The 21cm Power Spectrum at z=8.4Sep 25, 2019Mitigating Internal Instrument Coupling II: A Method Demonstration with the Hydrogen Epoch of Reionization ArrayOct 10, 2022Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I ObservationsApr 25, 2021Effects of model incompleteness on the drift-scan calibration of radio telescopesApr 23, 2020DAYENU: A Simple Filter of Smooth Foregrounds for Intensity Mapping Power SpectraFeb 2, 2026The Electromagnetically Isolated Global Signal Estimation Platform (EIGSEP)Jul 24, 2023The Impact of Beam Variations on Power Spectrum Estimation for 21 cm Cosmology II: Mitigation of Foreground Systematics for HERA