Simulations indicate HI absorption in FRB spectra is detectable when scintillation decorrelation bandwidth differs markedly from absorption width, with ≳1000 stacked bursts needed at current sensitivities.
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2 Pith papers cite this work, alongside 35 external citations. Polarity classification is still indexing.
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Kinematic distances for 66 pulsars are computed from archival HI radial velocities using a modern Galactic rotation curve and show agreement with independent parallax measurements within 1 sigma for nearly all objects with both.
citing papers explorer
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The Role of Scintillation in Detecting HI Absorption in FRB Spectra
Simulations indicate HI absorption in FRB spectra is detectable when scintillation decorrelation bandwidth differs markedly from absorption width, with ≳1000 stacked bursts needed at current sensitivities.
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Characterizing Pulsar Distances Using HI Kinematics
Kinematic distances for 66 pulsars are computed from archival HI radial velocities using a modern Galactic rotation curve and show agreement with independent parallax measurements within 1 sigma for nearly all objects with both.