High-Energy Emission from Pulsars and their Systems

By D. Torres, N. Rea. 2011

234 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Biomedical Engineering, Oceanography

View Paper: https://www.semanticscholar.org/paper/9ab9c86bb4f7f18ba8e19b334b139f544a0d56aa

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. D. R. Lorimer
2. S. Bates
3. E. Thrane
4. J. Verbiest
5. Marek Lewicki
6. John Ellis
7. G. Hobbs
8. V. Vaskonen

In Biomedical Engineering

1. D. R. Lorimer
2. S. Bates
3. J. Verbiest

In Oceanography

1. D. R. Lorimer
2. S. Bates
3. E. Thrane
4. J. Verbiest
5. Michela Mapelli
6. G. Hobbs

Citations in the corpus

• Be/X-ray binaries (2011, unknown): “As in the microquasar-jet models, the γ-ray emission can be produced by inverse Compton scattering of the relativistic particles from the pulsar wind on stellar photons (Torres 2010, and references therein).”
• The pulsar spectral index distribution (2013, methodology): “There are two main techniques which are commonly applied when simulating the pulsar population (for a recent review, see Lorimer 2011).”
• Sensitivity curves for searches for gravitational-wave backgrounds (2013, background): “1: Sensitivity curves for gravitational-wave observations and the predicted spectra of various gravitational-wave sources, taken from [1].”