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The cosmic gamma-ray background in the MeV range
P. Ruiz-Lapuente, M. Casse, E. Vangioni-Flam
The -ray background from supernovae is calculated on the basis of the reconstructed efficiency of supernova explosions from star formation at various redshifts. The calculations…
The very red afterglow of GRB 000418 - further evidence for dust extinction in a GRB host galaxy
S. Klose, B. Stecklum, N. Masetti +36
We report near-infrared and optical follow-up observations of the afterglow of the Gamma-Ray Burst 000418 starting 2.5 days after the occurrence of the burst and extending over nea…
The Discovery of an Embedded Cluster of High-Mass Stars Near SGR 1900+14
Frederick J. Vrba, Arne A. Henden, Christian B. Luginbuhl +3
Deep I-band imaging to approximately I = 26.5 of the soft gamma-ray repeater SGR 1900+14 region has revealed a compact cluster of massive stars located only a few arcseconds from t…