Gamma-ray haloes around pulsars as the key to understanding cosmic-ray transport in the Galaxy
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 …
pulsar, eventually permeating our Galaxy. The acceleration and propagation of these cosmic …
The HESS Galactic plane survey
We present the results of the most comprehensive survey of the Galactic plane in very high-
energy (VHE) γ-rays, including a public release of Galactic sky maps, a catalog of VHE …
energy (VHE) γ-rays, including a public release of Galactic sky maps, a catalog of VHE …
Gamma rays as probes of cosmic-ray propagation and interactions in galaxies
Continuum gamma-ray emission produced by interactions of cosmic rays with interstellar
matter and radiation fields is a probe of non-thermal particle populations in galaxies. After …
matter and radiation fields is a probe of non-thermal particle populations in galaxies. After …
Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre
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 …
to search for thermally produced dark matter at the TeV scale, via the associated gamma-ray …
Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth
The unexpectedly high flux of cosmic-ray positrons detected at Earth may originate from
nearby astrophysical sources, dark matter, or unknown processes of cosmic-ray secondary …
nearby astrophysical sources, dark matter, or unknown processes of cosmic-ray secondary …
Inference of the local interstellar spectra of cosmic-ray nuclei Z≤ 28 with the GalProp–HelMod framework
Composition and spectra of Galactic cosmic rays (CRs) are vital for studies of high-energy
processes in a variety of environments and on different scales, for interpretation of γ-ray and …
processes in a variety of environments and on different scales, for interpretation of γ-ray and …
HESS observations of RX J1713. 7− 3946 with improved angular and spectral resolution: Evidence for gamma-ray emission extending beyond the X-ray emitting shell
Supernova remnants exhibit shock fronts (shells) that can accelerate charged particles up to
very high energies. In the past decade, measurements of a handful of shell-type supernova …
very high energies. In the past decade, measurements of a handful of shell-type supernova …
Standardized and reproducible measurement of decision-making in mice
International Brain Laboratory, V Aguillon-Rodriguez… - Elife, 2021 - elifesciences.org
Progress in science requires standardized assays whose results can be readily shared,
compared, and reproduced across laboratories. Reproducibility, however, has been a …
compared, and reproduced across laboratories. Reproducibility, however, has been a …
Evidence of 100 TeV γ-ray emission from HESS J1702-420: A new PeVatron candidate
H Abdalla, F Aharonian, FA Benkhali… - Astronomy & …, 2021 - aanda.org
Aims. The identification of PeVatrons, hadronic particle accelerators reaching the knee of the
cosmic ray spectrum (few× 10 15 eV), is crucial to understand the origin of cosmic rays in the …
cosmic ray spectrum (few× 10 15 eV), is crucial to understand the origin of cosmic rays in the …
Characterising the VHE diffuse emission in the central 200 parsecs of our Galaxy with HESS
The diffuse very high-energy (VHE;> 100 GeV) γ-ray emission observed in the central 200
pc of the Milky Way by HESS was found to follow dense matter distribution in the central …
pc of the Milky Way by HESS was found to follow dense matter distribution in the central …