Constraining the cosmic ray spectrum in the vicinity of the supernova remnant W28: from sub-GeV to multi-TeV energies

We recorded the infrared spectrum of pyrene C 16 H 10 microcrystals embedded in a KBr pel- let over a wide range of temperature (14 -723 K) and studied the evolution of band

Pour un liquide plus léger que le solide, lorsque la cristallisation s’effectue depuis le bas vers le haut, la séparation de phase dans la zone de mush diminue l’épaisseur au sein

The workshops indicate that combining ModKit with the LilyPad ProtoSnap board is helpful in introducing computer science concepts to programming novices quickly and without

Les nouveaux développements portent sur l’étape locale de contact intégrant l’histoire du chargement, un critère de convergence adapté aux échelles considérées, le

In this section we mode the ejection of the VLBI component C13 assuming a single spinning BH, the VLBI ejection is perturbed by the precession of the accretion disk, and the

Qu’un Olympien avait lancé dans son jeune âge. Mélangeant

In the full Monte Carlo approach, because of the systematic uncertainties and the lack of knowledge of the mass composition of cosmic rays in this energy range, the spectrum has

c) (bottom right) To obtain the period one can study the power spectrum density of X and Y positions of photons detected on the imager. Here we show the periodogram, i.e. the