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High-Energy Emission from Pulsars and their Systems

M.-H. Grondin and M. Lemoine-Goumard
Astrophysics and Space Science Proceedings, High-Energy Emission from Pulsars and their Systems 399 (2011)
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Associations of very high energy gamma-ray sources discovered by H.E.S.S. with pulsar wind nebulae

Yves A. Gallant
Astrophysics and Space Science 309 (1-4) 197 (2007)
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Astrophysical limits on Lorentz violation for all charged species

Brett Altschul
Astroparticle Physics 28 (3) 380 (2007)
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X-RAY EVOLUTION OF PULSAR WIND NEBULAE

Aya Bamba, Takayasu Anada, Tadayasu Dotani, et al.
The Astrophysical Journal 719 (2) L116 (2010)
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Search for PeV Gamma-Ray Emission from the Southern Hemisphere with 5 Yr of Data from the IceCube Observatory

M. G. Aartsen, M. Ackermann, J. Adams, et al.
The Astrophysical Journal 891 (1) 9 (2020)
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IN TE G R AL IGR J18135-1751 = HESS J1813-178: A New Cosmic High-Energy Accelerator from keV to TeV Energies

P. Ubertini, L. Bassani, A. Malizia, et al.
The Astrophysical Journal 629 (2) L109 (2005)
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High-Energy Particles in the Wind Nebula of Pulsar B1509-58 as Seen by INTEGRAL

M. Forot, W. Hermsen, M. Renaud, et al.
The Astrophysical Journal 651 (1) L45 (2006)
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PSR J1856+0245: Arecibo Discovery of a Young, Energetic Pulsar Coincident with the TeV γ-Ray Source HESS J1857+026

J. W. T. Hessels, D. J. Nice, B. M. Gaensler, et al.
The Astrophysical Journal 682 (1) L41 (2008)
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The H.E.S.S. Galactic plane survey

H. Abdalla, A. Abramowski, F. Aharonian, et al.
Astronomy & Astrophysics 612 A1 (2018)
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Multiband nonthermal radiative properties of pulsar wind nebulae

Bo-Tao Zhu, Li Zhang and Jun Fang
Astronomy & Astrophysics 609 A110 (2018)
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Search for continuous gravitational waves from ten H.E.S.S. sources using a hidden Markov model

Deeksha Beniwal, Patrick Clearwater, Liam Dunn, Andrew Melatos and David Ottaway
Physical Review D 103 (8) (2021)
DOI: 10.1103/PhysRevD.103.083009
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Improved Bounds on Lorentz Symmetry Violation from High-Energy Astrophysical Sources

Brett Altschul
Symmetry 13 (4) 688 (2021)
DOI: 10.3390/sym13040688
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