FRB 190523 is localized to a massive galaxy at z=0.66, a thousand times more massive and with over 100 times lower specific star-formation rate than the dwarf galaxy host of FRB 121102.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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astro-ph.HE 2years
2019 2representative citing papers
Volumetric rate of non-repeating FRBs exceeds candidate one-off progenitor rates, implying most FRBs originate from repeating sources.
citing papers explorer
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A fast radio burst localised to a massive galaxy
FRB 190523 is localized to a massive galaxy at z=0.66, a thousand times more massive and with over 100 times lower specific star-formation rate than the dwarf galaxy host of FRB 121102.
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The prevalence of repeating fast radio bursts
Volumetric rate of non-repeating FRBs exceeds candidate one-off progenitor rates, implying most FRBs originate from repeating sources.