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laboratory facilities. More specifically TEC-EF responsibilities encompass at subsystem and instrument level: Payloads with RF interface exploiting different technologies (e.g., analogue, digital, optical
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laboratory facilities. More specifically TEC-EF responsibilities encompass at subsystem and instrument level: Payloads with RF interface exploiting different technologies (e.g., analogue, digital, optical
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laboratory facilities. More specifically TEC-EF responsibilities encompass at subsystem and instrument level: Payloads with RF interface exploiting different technologies (e.g., analogue, digital, optical
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diffraction components. As antenna dimensions scale with wavelength, the number or antennas and the way to integrate them in transceivers also differs a lot. This requires investigating the most appropriate
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develop advanced signal processing techniques that empower a single UWB multi-antenna radio platform to perform all these functions concurrently, significantly enhancing the situational awareness and
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target is observed by a different portion of the azimuth antenna pattern. This effect along with an antenna beam mispointing causes a periodic modulation of the image radiometry and a variation of the
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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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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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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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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