Automated Detection of Antenna Malfunctions in Large-N Interferometers: A Case Study with the Hydrogen Epoch of Reionization Array
arXiv:2109.12733 · doi:10.1029/2021RS007376
Abstract
We present a framework for identifying and flagging malfunctioning antennas in large radio interferometers. We outline two distinct categories of metrics designed to detect outliers along known failure modes of large arrays: cross-correlation metrics, based on all antenna pairs, and auto-correlation metrics, based solely on individual antennas. We define and motivate the statistical framework for all metrics used, and present tailored visualizations that aid us in clearly identifying new and existing systematics. We implement these techniques using data from 105 antennas in the Hydrogen Epoch of Reionization Array (HERA) as a case study. Finally, we provide a detailed algorithm for implementing these metrics as flagging tools on real data sets.
arXiv comment31 pages, 17 figures
References in corpus (28)
- LOFAR: The LOw-Frequency ARray
- Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
- The Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies
- 21-cm cosmology
- Hydrogen Epoch of Reionization Array (HERA)
- Reionization and Cosmology with 21 cm Fluctuations
- The Precision Array for Probing the Epoch of Reionization: 8 Station Results
- Reionization and the Cosmic Dawn with the Square Kilometre Array
- Data Analysis for Precision 21 cm Cosmology
- Systematic effects in LOFAR data: A unified calibration strategy
- First Results from HERA Phase I: Upper Limits on the Epoch of Reionization 21 cm Power Spectrum
- The GMRT-EoR Experiment: A new upper limit on the neutral hydrogen power spectrum at z~8.6
- Design and characterization of the Large-Aperture Experiment to Detect the Dark Age (LEDA) radiometer systems
- First Season MWA EoR Power Spectrum Results at Redshift 7
- Foregrounds for observations of the cosmological 21 cm line: II. Westerbork observations of the fields around 3C196 and the North Celestial Pole
- Mitigating Internal Instrument Coupling for 21 cm Cosmology I: Temporal and Spectral Modeling in Simulations
- Mitigating Internal Instrument Coupling II: A Method Demonstration with the Hydrogen Epoch of Reionization Array
- Redundant Array Configurations for 21 cm Cosmology
- Redundant-Baseline Calibration of the Hydrogen Epoch of Reionization Array
- Absolute Calibration Strategies for the Hydrogen Epoch of Reionization Array and Their Impact on the 21 cm Power Spectrum
- The Hydrogen Epoch of Reionization Array Dish II: Characterization of Spectral Structure with Electromagnetic Simulations and its science Implications
- Quantifying Excess Power from Radio Frequency Interference in Epoch of Reionization Measurements
- A Map of Diffuse Radio Emission at 182 MHz to Enhance Epoch of Reionization Observations in the Southern Hemisphere
- A First Search for Prompt Radio Emission from a Gravitational-Wave Event
- Dual Polarization Measurements of MWA Beampatterns at 137 MHz
- Packed Ultra-wideband Mapping Array (PUMA): Astro2020 RFI Response
- Van Vleck correction generalization for complex correlators with multilevel quantization
- Epoch of Reionization Power Spectrum Limits from Murchison Widefield Array Data Targeted at EoR1 Field