Reanalysis of pulsar data shows polarization angles in PSRs B1133+16 and B2016+28 follow great-circle geodesics on the Poincare sphere due to mode transitions.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.HE 2years
2026 2representative citing papers
PATH is extended with three fitted P(m_r|z) prior models combined with P(z|DM), raising host-association confidence for ASKAP FRBs while showing fainter-than-expected host magnitude distribution.
citing papers explorer
-
Polarization Angle Geodesics in PSRs B1133+16 and B2016+28
Reanalysis of pulsar data shows polarization angles in PSRs B1133+16 and B2016+28 follow great-circle geodesics on the Poincare sphere due to mode transitions.
-
Updating the PATH framework with FRB host galaxy models
PATH is extended with three fitted P(m_r|z) prior models combined with P(z|DM), raising host-association confidence for ASKAP FRBs while showing fainter-than-expected host magnitude distribution.