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Characterising radio sources in the Small Magellanic Cloud using citizen science and optical spectroscopy
For several years, the Small Magellanic Cloud (SMC) has been extensively studied in multiple wavelengths, revealing rich populations of radio sources within and beyond the nearby dwarf galaxy. With radio interfer-ometers' ever-increasing sensitivity and resolution, greater source populations will be...
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| Language: | English English |
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Department of Astronomy
2025
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