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network aims to deliver fiber-optic quality experiences over wireless links by building the theoretical, algorithmic, and architectural foundations of THz systems. It introduces ultra-MIMO (multiple-input
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, the Laser Interferometer Space Antenna (LISA) will begin to observe thousands of low-frequency gravitational-wave sources, including ultracompact stellar-remnant binaries in the Milky Way, and the mergers
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Archipelago, integrating it into the global e-CALLISTO network. The project will deploy new-generation spectrometers and antennas to fill the observational gap over the North Atlantic, enhancing global space
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processing algorithms for joint communication and sensing. Analyze experimental datasets, extract statistical models, and compare findings across environments, hardware, and frequency bands. Collaborate with
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goals As a researcher in this project, you will work on mathematical models for describing the radio environment and to design algorithms for estimating, for example, the location and spectral
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RF front-ends (FR2, FR3, V-band) into end-to-end ISAC demonstrators. Implement and optimize advanced signal processing algorithms for joint communication and sensing. Analyze experimental datasets
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establishing the existence of binaries of stellar-mass black holes. In the mid-2030s, the Laser Interferometer Space Antenna (LISA) will begin to observe thousands of low-frequency gravitational-wave sources
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in signal processing and control. Your role and goals As a researcher in this project, you will work on mathematical models for describing the radio environment and to design algorithms for estimating
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, and fine-grained sensing. In this PhD project, you will develop advanced signal processing techniques that empower a single UWB multi-antenna radio platform to perform all these functions concurrently
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on Antennas and Propagation, Volume 61(3): 1285, 2013 Gimbutas Z, Greengard L: Journal of Computational Physics 232: 22, 2013. doi:http://dx.doi.0rg10.1016/jjcp.2012.01.041, arXiv:1104.5293v1 key words