Quantifying Foreground Contamination in the Dark Ages 21 cm Power Spectrum Using an Electromagnetically Simulated Dipole Antenna Atop a Dielectric Surface
Willow Smith, Jonathan C. Pober, Bang D. Nahn, Jack O. Burns, Ronald S. Polidan
astro-ph.IM, astro-ph.CO
Submitted: 2026-07-10
Comments: 14 pages, 9 figures
Code: https://github.com/aelanman/lunarsky
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- LuSEE 'Night': The Lunar Surface Electromagnetics Experiment
- The Dark Ages Explorer (DEX): a filled-aperture ultra-long wavelength radio interferometer on the lunar far side
- Global 21-cm Cosmology from the Farside of the Moon
- The FarView Low Frequency Radio Array on the Moon's Far Side: Science and Array Architecture
- Peering into the Dark (Ages) with Low-Frequency Space Interferometers
- Complete Sampling of the $uv$ Plane with Realistic Radio Arrays: Introducing the RULES Algorithm, with Application to 21 cm Foreground Wedge Removal
- The Impact of Foregrounds on Dark Ages Measurements with the Highly Redshifted 21 cm Line
- FarView: An In-Situ Manufactured Lunar Far Side Radio Array Concept for 21-cm Dark Ages Cosmology
- Electrical coupling of a horizontal dipole antenna to a dielectric half-space: applications to radio astronomy from the lunar surface
- Detecting the 21 cm Signal of the Cosmic Dark Ages
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