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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3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
representative citing papers
UVJ colors saturate below log(sSFR) ~ -10.5; new UV/MIR color-color diagrams allow more efficient selection of galaxies with substantially lower ongoing star formation.
Star formation histories inferred for z=2-5 massive quiescent galaxies imply past number densities that align with observed rapid evolution since z~7.
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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Beyond UVJ: More Efficient Selection of Quiescent Galaxies With UV / Mid-IR Fluxes
UVJ colors saturate below log(sSFR) ~ -10.5; new UV/MIR color-color diagrams allow more efficient selection of galaxies with substantially lower ongoing star formation.
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Winding Back the Clock: Recent Star Formation Histories of Massive Quiescent Galaxies Are Consistent With Their Rapid Number Density Evolution Since $\mathbf{z\sim7}$
Star formation histories inferred for z=2-5 massive quiescent galaxies imply past number densities that align with observed rapid evolution since z~7.