X-ray polarization of 13.1% ± 3.0% is detected from LS I +61 303 at 4.2 sigma, with EVPA alignment to the binary axis depending on which set of orbital elements is adopted.
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2 Pith papers cite this work. Polarity classification is still indexing.
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TeV-selected PWNe and unidentified sources yield beaming fractions of 0.1-0.3 across radio, gamma-ray, and X-ray bands, with survey-to-survey differences explained by selection biases or older pulsars and reproducible via time-dependent opening angles.
citing papers explorer
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X-Ray Polarization from the Gamma-Ray Binary LS I +61 303
X-ray polarization of 13.1% ± 3.0% is detected from LS I +61 303 at 4.2 sigma, with EVPA alignment to the binary axis depending on which set of orbital elements is adopted.
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Constraining the Pulsar Beaming Fraction with TeV-Selected Galactic Pulsar Wind Nebulae and unidentified TeV Sources
TeV-selected PWNe and unidentified sources yield beaming fractions of 0.1-0.3 across radio, gamma-ray, and X-ray bands, with survey-to-survey differences explained by selection biases or older pulsars and reproducible via time-dependent opening angles.