VERITAS and multiwavelength observations of the 2017 NGC 1275 gamma-ray flare show harder-when-brighter spectral evolution and support a two-component jet model with 10-degree viewing angle and gamma-ray emission near the C3 radio component.
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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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The exceptional 2017 gamma-ray flare of the radio galaxy NGC 1275: VERITAS and Multiwavelength Observations
VERITAS and multiwavelength observations of the 2017 NGC 1275 gamma-ray flare show harder-when-brighter spectral evolution and support a two-component jet model with 10-degree viewing angle and gamma-ray emission near the C3 radio component.
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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.