Abstract The Alpha Magnetic Spectrometer (AMS) is a precision particle physics detector on
the International Space Station (ISS) conducting a unique, long-duration mission of …

Pulsars are factories of relativistic electrons and positrons that propagate away from the
pulsar, eventually permeating our Galaxy. The acceleration and propagation of these cosmic …

Precision measurements of cosmic ray positrons are presented up to 1 TeV based on 1.9
million positrons collected by the Alpha Magnetic Spectrometer on the International Space …

We report the discovery of an extended very-high-energy (VHE) gamma-ray source around
the location of the middle-aged (207.8 kyr) pulsar PSR J 0622+ 3749 with the Large High …

Weakly interacting massive particles (WIMPs) have long reigned as one of the leading
classes of dark matter candidates. The observed dark matter abundance can be naturally …

The past decade has brought impressive advances in the astrophysics of cosmic rays (CRs)
and multiwavelength astronomy, thanks to the new instrumentation launched into space and …

Precision results on cosmic-ray electrons are presented in the energy range from 0.5 GeV to
1.4 TeV based on 28.1× 10 6 electrons collected by the Alpha Magnetic Spectrometer on the …

The HAWC Collaboration has discovered a γ-ray emission extended about 2 degrees
around the Geminga and Monogem pulsar wind nebulae (PWNe) at γ-ray energies E γ> 5 …

Context. The vertical diffusive halo size of the Galaxy, L, is a key parameter for dark matter
indirect searches. It can be better determined thanks to recent AMS-02 data. Aims. We set …

Milagro and the High Altitude Water Cherenkov (HAWC) observatory have detected
extended TeV gamma-ray emission around nearby pulsar wind nebulae. Building on these …