The aim of the inaugural meeting of the Sant Cugat Forum on
Astrophysics was to address, in a global context, the current
understanding of and challenges in high-energy emissions from
isolated and non-isolated neutron stars, and to confront the
theoretical picture with observations of both the Fermi satellite
and the currently operating ground-based Cherenkov telescopes.
Participants have also discussed the prospects for possible
observations with planned instruments across the multi-wavelength
spectrum (e.g. SKA, LOFAR, E-VLT, IXO, CTA) and how they will
impact our theoretical understanding of these systems.
In keeping with the goals of the Forum, this book not only
represents the proceedings of the meeting, but also a reflection on
the state-of-the-art in the topic.
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