Drone Beam Mapping of the TONE Radio Dish Array
arXiv:2502.03759 · doi:10.3847/1538-3881/add269
Abstract
Drone-based beam measurements are a promising avenue to tackle the critical challenge of calibration for 21 cm cosmology telescopes. In this paper, we introduce a new drone-based calibration system for 400-800 MHz radio observatories, describing its instrumentation and first deployment. We discuss measurements of the TONE array, a CHIME/FRB outrigger pathfinder, and present results, including full 2D high spatial resolution beam maps in both co- and cross-polarization, as well as comparisons to simulations. The polarized beam maps cover a 70 degree by 70 degree grid, capturing the first two sidelobes and measuring the TONE main beam and first sidelobe with 7-9% statistical errors. We investigate polarization angle alignment with frequency, finding significant polarization leakage in the TONE antennas at frequencies above 600 MHz, and a polarization axis rotation with frequency. We describe statistical and systematic errors, as well as measurements of radio frequency interference from the drone and equipment. Our drone system is the first to incorporate a broad-band switched calibration source in the drone payload, enabling background subtraction and direct measurements of the RFI emitted by the drone. The results presented are the first drone-based 2D measurements of cross-polar beam structure and of polarization alignment of an array. The high frequency and spatial resolution achieved with this system have revealed the rich structure of the beam of each antenna, and enabled comparisons between individual dishes and to electromagnetic simulations.
26 Pages, 19 Figures, 4 Tables. This is a pre-copyedited, author-produced PDF of an article accepted for publication in The Astronomical Journal following peer review (2025 July). The version of record is available online at: https://iopscience.iop.org/article/10.3847/1538-3881/add269
References in corpus (24)
- LOFAR: The LOw-Frequency ARray
- The Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies
- Hydrogen Epoch of Reionization Array (HERA)
- Bright Source Subtraction Requirements For Redshifted 21 cm Measurements
- A Per-Baseline, Delay-Spectrum Technique for Accessing the 21cm Cosmic Reionization Signature
- Toward Epoch of Reionization Measurements with Wide-Field Radio Observations
- Data Analysis for Precision 21 cm Cosmology
- A Method for 21cm Power Spectrum Estimation in the Presence of Foregrounds
- Coaxing Cosmic 21cm Fluctuations from the Polarized Sky using m-mode Analysis
- HIRAX: A Probe of Dark Energy and Radio Transients
- Foregrounds in Wide-Field Redshifted 21 cm Power Spectra
- Foregrounds for 21cm Observations of Neutral Gas at High Redshift
- The 21 centimeter emission from the reionization epoch: extended and point source foregrounds
- LRP 2020 Whitepaper: The Canadian Hydrogen Observatory and Radio-transient Detector (CHORD)
- Beam calibration of radio telescopes with drones
- DAYENU: A Simple Filter of Smooth Foregrounds for Intensity Mapping Power Spectra
- The BINGO telescope: a new instrument exploring the new 21-cm cosmology window
- The cloverleaf antenna: A compact wide-bandwidth dual-polarization feed for CHIME
- Measuring HERA's primary beam in-situ: methodology and first results
- Beam Measurements of the Tianlai Dish Radio Telescope using an Unmanned Aerial Vehicle
- Using the Sun to Measure the Primary Beam Response of the Canadian Hydrogen Intensity Mapping Experiment
- Dual Polarization Measurements of MWA Beampatterns at 137 MHz
- Holographic Beam Measurements of the Canadian Hydrogen Intensity Mapping Experiment (CHIME)
- TONE: A CHIME/FRB Outrigger Pathfinder for localizations of Fast Radio Bursts using Very Long Baseline Interferometry