Starlink DTC satellites show reversed solar illumination dependence in unintended emissions at 72-234 MHz, brighter in eclipse than sunlight unlike Ku-only satellites, pointing to an active on-board source.
Tingay and Raunaq Bhushan and Tom Booler and Riccardo Chiello and David B
2 Pith papers cite this work. Polarity classification is still indexing.
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abstract
We present the Engineering Development Array 2, which is one of two instruments built as a second generation prototype station for the future Square Kilometre Array Low Frequency Array. The array is comprised of 256 dual-polarization dipole antennas that can work as a phased array or as a standalone interferometer. We describe the design of the array and the details of design changes from previous generation instruments, as well as the motivation for the changes. Using the array as an imaging interferometer, we measure the sensitivity of the array at five frequencies ranging from 70 to 320 MHz.
years
2026 2representative citing papers
Atlas of 205 non-recycled southern pulsars at 140–170 MHz from MWA SMART data, with profiles, DMs, RMs, fluxes and public data products for SKA-Low.
citing papers explorer
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A reversed solar illumination dependence of unintended emission from Starlink Direct-to-Cell satellites at 72-234 MHz with the EDA2
Starlink DTC satellites show reversed solar illumination dependence in unintended emissions at 72-234 MHz, brighter in eclipse than sunlight unlike Ku-only satellites, pointing to an active on-board source.
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The Southern-sky MWA Rapid Two-metre (SMART) pulsar survey--IV. Survey update and an atlas of 205 non-recycled southern pulsars
Atlas of 205 non-recycled southern pulsars at 140–170 MHz from MWA SMART data, with profiles, DMs, RMs, fluxes and public data products for SKA-Low.