The Review summarizes much of particle physics and cosmology. Using data from previous
editions, plus 2,143 new measurements from 709 papers, we list, evaluate, and average�…

On the 15th of June 2006, the PAMELA (Payload for Antimatter Matter Exploration and Light-
nuclei Astrophysics) satellite-borne experiment was launched onboard the Russian Resurs�…

Neutrino astronomy beyond the Sun was first imagined in the late 1950s; by the 1970s, it
was realized that kilometer-scale neutrino detectors were required. The first such instrument�…

Abstract The Crab Nebula is the brightest TeV gamma-ray source in the sky and has been
used for the past 25 years as a reference source in TeV astronomy, for calibration and�…

We provide an updated assessment of the power of the Cherenkov Telescope Array (CTA)
to search for thermally produced dark matter at the TeV scale, via the associated gamma-ray�…

Weakly interacting massive particles (WIMPs) are a theoretical class of particles that are
excellent dark matter candidates. WIMP annihilation or decay may produce essentially�…

Abstract The High Altitude Water Cherenkov (HAWC) observatory is an array of large water
Cherenkov detectors sensitive to gamma rays and hadronic cosmic rays in the energy band�…

Recent observations by PAMELA, Fermi-LAT, and AMS-02 have conclusively indicated a
rise in the cosmic-ray positron fraction above 10 GeV, a feature which is impossible to mimic�…

In the last few decades, a number of experiments have provided long-term, statistically
significant evidence of a faint sidereal anisotropy in the cosmic-ray arrival direction�…

We report the first observation of an anisotropy in the arrival direction of cosmic rays with
energies in the multi-TeV region in the Southern sky using data from the IceCube detector�…