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.
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HAWC observations of Mrk 421 reveal a 13±3 TeV cutoff in high states at 3.8σ significance, indicating intrinsic origin and providing EBL intensity upper limits.
citing papers explorer
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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.
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Constraining the Photon Intensity of Extragalactic Background Light with the HAWC Observatory for the Blazar Mrk 421
HAWC observations of Mrk 421 reveal a 13±3 TeV cutoff in high states at 3.8σ significance, indicating intrinsic origin and providing EBL intensity upper limits.