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Testbed Evaluation of Distributed Radio Timing Alignment Over Ethernet Fronthaul Networks
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Genèse de la BBC ou les balbutiements de sa Majesté des ondes
Published 2020-12-01Subjects: Get full text
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Digitising Context
Published 2012-02-01“…There will also be descriptions about these programmes as reflected in the Radio Times and information on the contributors, performers, directors and producers.…”
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THE OLIVETTI CHRONICLES : Three Decades of Life and Music /
Published 2009“…He wrote articles, columns, and reviews for publications as diverse as The Listener, Oz, Gandalf's Garden, Sounds, the Observer, the Independent, and Radio Times. Now for the first time, the best of these writings have been brought together—selected by his wife, Sheila, and his four children. …”
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Robust time synchronization for NC-OFDM cognitive radio systems
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BEATING THE SPIN-DOWN LIMIT ON GRAVITATIONAL WAVE EMISSION FROM THE VELA PULSAR
Published 2015“…These upper limits have been obtained using three independent methods that assume the gravitational wave emission follows the radio timing. Two of the methods produce frequentist upper limits for an assumed known orientation of the star's spin axis and value of the wave polarization angle of, respectively, 1.9 × 10–24 and 2.2 × 10–24, with 95% confidence. …”
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Decade-long Timing Study of the Black Widow Millisecond Pulsar J1544+4937
Published 2023-01-01“…Results from 11 yr of radio timing for the eclipsing black widow millisecond pulsar (MSP) binary J1544+4937 is presented in this paper. …”
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An <italic>In Vitro</italic> Experimental System for 5G 3.5 GHz Exposures
Published 2022-01-01“…A 5G signal generator along with a customized power amplifier can create 5G new radio time division duplex (TDD) waveforms. Additionally, a feedback scheme implemented by employing a directional coupler and power meter allows power control to ensure a steady output power. …”
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On the nature and evolution of the unique binary pulsar J1903+0327
Published 2010“…Here we describe optical and radio observations which rule out most of the scenarios proposed to explain formation of this system. Radio timing measurements of three post-Keplerian effects yield the most precise measurement of the mass of a millisecond pulsar to date: 1.667 +/- 0.021 solar masses (99.7% confidence limit) (...). …”
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