Optimized Beam Sculpting with Generalized Fringe-Rate Filters
arXiv:1503.05564 · doi:10.3847/0004-637X/820/1/51
Abstract
We generalize the technique of fringe-rate filtering, whereby visibilities measured by a radio interferometer are re-weighted according to their temporal variation. As the Earth rotates, radio sources traverse through an interferometer's fringe pattern at rates that depend on their position on the sky. Capitalizing on this geometric interpretation of fringe rates, we employ time-domain convolution kernels to enact fringe-rate filters that sculpt the effective primary beam of antennas in an interferometer. As we show, beam sculpting through fringe-rate filtering can be used to optimize measurements for a variety of applications, including mapmaking, minimizing polarization leakage, suppressing instrumental systematics, and enhancing the sensitivity of power-spectrum measurements. We show that fringe-rate filtering arises naturally in minimum variance treatments of many of these problems, enabling optimal visibility-based approaches to analyses of interferometric data that avoid systematics potentially introduced by traditional approaches such as imaging. Our techniques have recently been demonstrated in Ali et al. (2015), where new upper limits were placed on the 21 cm power spectrum from reionization, showcasing the ability of fringe-rate filtering to successfully boost sensitivity and reduce the impact of systematics in deep observations.
18 pages, 9 figures. Revised to match accepted ApJ version; minor editorial changes throughout, with no change to results
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- PAPER-64 Constraints on Reionization: The 21cm Power Spectrum at z=8.4
- Data Analysis for Precision 21 cm Cosmology
- First Results from HERA Phase I: Upper Limits on the Epoch of Reionization 21 cm Power Spectrum
- Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I Observations
- A simplified, lossless re-analysis of PAPER-64
- First Limits on the 21 cm Power Spectrum during the Epoch of X-ray heating
- Mitigating Internal Instrument Coupling for 21 cm Cosmology I: Temporal and Spectral Modeling in Simulations
- Characterizing Signal Loss in the 21 cm Reionization Power Spectrum: A Revised Study of PAPER-64
- Understanding the Diversity of 21 cm Cosmology Analyses
- Spherical Harmonic Analyses of Intensity Mapping Power Spectra
- A 21-cm power spectrum at 48 MHz, using the Owens Valley Long Wavelength Array
- Absolute Calibration Strategies for the Hydrogen Epoch of Reionization Array and Their Impact on the 21 cm Power Spectrum
- Polarized Redundant-Baseline Calibration for 21 cm Cosmology Without Adding Spectral Structure
- Constraints on the temperature of the intergalactic medium at z=8.4 with 21-cm observations
- Array Element Coupling in Radio Interferometry I: A Semi-Analytic Approach
- Precision requirements for interferometric gridding in 21-cm power spectrum analysis
- Validation of the HERA Phase I Epoch of Reionization 21 cm Power Spectrum Software Pipeline
- Extracting the 21 cm EoR signal using MWA drift scan data
- A Bayesian analysis of redshifted 21-cm HI signal and foregrounds: Simulations for LOFAR
- The Impact of Beam Variations on Power Spectrum Estimation for 21-cm Cosmology I: Simulations of Foreground Contamination for HERA
- Methods of Error Estimation for Delay Power Spectra in Cosmology
- Using baseline-dependent window functions for data compression and field-of-interest shaping in radio interferometry
- On the use of temporal filtering for mitigating galactic synchrotron calibration bias in 21 cm reionization observations
- Baseline-dependent sampling and windowing for radio interferometry: data compression, field-of-interest shaping and outer field suppression
- Why and When to Expect Gaussian Error Distributions in Epoch of Reionization 21-cm Power Spectrum Measurements
- A Differentiable, End-to-End Forward Model for 21 cm Cosmology: Estimating the Foreground, Instrument, and Signal Joint Posterior
- The Tracking Tapered Gridded Estimator (TTGE) for the power spectrum from drift scan observations
- Detecting 21 cm EoR Signal using Drift Scans: Correlation of Time-ordered Visibilities