Showing 1–19 of 19 results
/ Date/ Name
Oct 8, 2025Stacking 21-cm Maps around Lyman-$α$ Emitters during Reionization: Prospects for a Cross-correlation Detection with the Hydrogen Epoch of Reionization ArrayNov 15, 2024Impacts and Statistical Mitigation of Missing Data on the 21cm Power Spectrum: A Case Study with the Hydrogen Epoch of Reionization ArrayJan 9, 2024Hydrogen Epoch of Reionization Array (HERA) Phase II Deployment and CommissioningDec 6, 2023Bayesian estimation of cross-coupling and reflection systematics in 21cm array visibility dataOct 10, 2022Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I ObservationsApr 12, 2022Direct Optimal Mapping for 21cm Cosmology: A Demonstration with the Hydrogen Epoch of Reionization ArrayMar 17, 2021Methods of Error Estimation for Delay Power Spectra in $21\,\textrm{cm}$ CosmologyMay 25, 2020Measuring HERA's primary beam in-situ: methodology and first resultsOct 28, 2019Absolute Calibration Strategies for the Hydrogen Epoch of Reionization Array and Their Impact on the 21 cm Power SpectrumSep 25, 2019Mitigating Internal Instrument Coupling II: A Method Demonstration with the Hydrogen Epoch of Reionization ArrayAug 6, 2019Understanding the HERA Phase I receiver system with simulations and its impact on the detectability of the EoR delay power spectrumJul 15, 2019A Roadmap for Astrophysics and Cosmology with High-Redshift 21 cm Intensity MappingMay 2, 2018HI 21cm Cosmology and the Bi-spectrum: Closure Diagnostics in Massively Redundant Interferometric ArraysJan 12, 2017The Hydrogen Epoch of Reionization Array Dish III: Measuring Chromaticity of Prototype Element with ReflectometryJun 23, 2016Hydrogen Epoch of Reionization Array (HERA)Jul 17, 2014Study of Redshifted HI from the Epoch of Reionization with Drift scanAug 2, 2013A study of fundamental limitations to statistical detection of redshifted HI from the epoch of reionizationDec 20, 2012Science with the Murchison Widefield ArrayMar 26, 2012Low Frequency Imaging of Fields at High Galactic Latitude with the Murchison Widefield Array 32-Element Prototype