VLBI confirms a compact non-thermal persistent radio source for FRB 20190417A with nearly flat spectrum α=-0.19±0.29, placing it on the Lν-|RM| relation consistent with young nebulae or forward shocks.
D., Ravi, V ., Belov, K
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No radio emission detected from 13 radio quiet magnetars with MeerKAT, providing upper limits of 60 μJy mean flux density and 39 mJy single-pulse fluence.
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The VLBI spectrum of the persistent radio source associated with FRB 20190417A
VLBI confirms a compact non-thermal persistent radio source for FRB 20190417A with nearly flat spectrum α=-0.19±0.29, placing it on the Lν-|RM| relation consistent with young nebulae or forward shocks.
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Searching for radio emission from radio quiet magnetars with MeerKAT
No radio emission detected from 13 radio quiet magnetars with MeerKAT, providing upper limits of 60 μJy mean flux density and 39 mJy single-pulse fluence.