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Intelligent Cognitive Radio Models for Enhancing Future Radio Astronomy Observations
Published 2016-01-01“…Radio astronomy organisations desire to optimise the terrestrial radio astronomy observations by mitigating against interference and enhancing angular resolution. …”
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Effect of Parasitic Element on 408 MHz Antenna for Radio Astronomy Application
Published 2014-01-01Get full text
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Optimization of a Conical Corrugated Antenna Using Multiobjective Heuristics for Radio-Astronomy Applications
Published 2016-01-01“…This paper presents the design of a tree sections corrugated horn antenna with a modified linear profile, using NURBS, suitable for radio-astronomy applications. The operating band ranges from 4.5 to 8.8 GHz. …”
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The Observed Phase Space of Mass-loss History from Massive Stars Based on Radio Observations of a Large Supernova Sample
Published 2025-01-01Subjects: Get full text
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Constraining Solar Emission Radius at 42 MHz During the 2024 Total Solar Eclipse Using a Student-commissioned Radio Telescope
Published 2025-01-01Subjects: “…Radio astronomy…”
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Deep Searches for Radio Pulsations and Bursts from Four Magnetar and a Magnetar-like Pulsar with FAST
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WALLABY Pilot Survey: Star Formation Enhancement and Suppression in Gas-rich Galaxy Pairs
Published 2025-01-01Get full text
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Fermi Unassociated Sources in the MeerKAT Absorption Line Survey
Published 2025-01-01Get full text
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WALLABY Pilot Survey and ASymba: Comparing H i Detection Asymmetries to the SIMBA Simulation
Published 2025-01-01Get full text
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Investigating the Source of Planck-Detected AME: High-Resolution Observations at 15 GHz
Published 2013-01-01Get full text
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Electromagnetic Analysis and Experimental Validation of the LOFAR Radiation Patterns
Published 2019-01-01“…Low-frequency (<300 MHz) aperture array systems are one of the new trends in modern radio astronomy. Among the challenges they pose, the instrumental calibration is a key aspect requiring an accurate and reliable model of each element of such electrically large array. …”
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Molecular Distributions and Abundances in the Binary-shaped Outflow of V Hya
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