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Fermi Observations of High-Energy Gamma-Ray Emission from GRB 080916C
TLDR
The Gamma-ray Burst Monitor and Large Area Telescope onboard the Fermi Observatory together record GRBs over a broad energy range spanning about 7 decades of gammaray energy, with the largest apparent energy release yet measured. Expand
THE CRYSTAL BALL COLLABORATION
The reaction e+e-+e+e-7r07r0 has been analyzed using 97 pb-’ of data taken with the Crystal Ball detector at the DORIS II e+estorage ring at beam energies around 5.3 GeV. For the first time we haveExpand
Photodestruction of hydrogen molecules in H I regions.
Photodissociation of hydrogen molecules in H I regions of interstellar medium, evaluating lifetime and density
TeV Gamma-ray Sources from a survey of the Galactic Plane with Milagro
A survey of Galactic gamma-ray sources at a median energy of ~20 TeV has been performed using the Milagro Gamma-Ray Observatory. Eight candidate sources of TeV emission are detected with pretrialExpand
THE FIRM REDSHIFT LOWER LIMIT OF THE MOST DISTANT TeV-DETECTED BLAZAR PKS 1424+240
We present the redshift lower limit of z ≥ 0.6035 for the very high energy (VHE; E ≥ 100 GeV) emitting blazar PKS 1424+240 (PG 1424+240). This limit is inferred from Lyβ and Lyγ absorption observedExpand
Discovery of TeV Gamma-Ray Emission from the Cygnus Region
The diffuse gamma radiation arising from the interaction of cosmic ray particles with matter and radiation in the Galaxy is one of the few probes available to study the origin of the cosmic rays.Expand
DISCOVERY OF TeV GAMMA-RAY EMISSION FROM TYCHO’S SUPERNOVA REMNANT
We report the discovery of TeV gamma-ray emission from the Type Ia supernova remnant (SNR) G120.1+1.4, known as Tycho's SNR. Observations performed in the period 2008-2010 with the VERITASExpand
Evaporation of ices near massive stars: models based on laboratory temperature programmed desorption data
Hot cores and their precursors contain an integrated record of the physics of the collapse process in the chemistry of the ices deposited during that collapse. In this paper, we present results fromExpand
Detection of Pulsed Gamma Rays Above 100 GeV from the Crab Pulsar
TLDR
This detection constrains the mechanism and emission region of gamma-ray radiation in the pulsar’s magnetosphere and requires that these gamma rays be produced more than 10 stellar radii from the neutron star. Expand
Radio imaging of the very-high-energy gamma-ray emission region in the central engine of a radio galaxy.
TLDR
Radio and VHE observations of the radio galaxy Messier 87 are revealed, revealing a period of extremely strong VHE gamma-ray flares accompanied by a strong increase of theRadio flux from its nucleus, implying that charged particles are accelerated to very high energies in the immediate vicinity of the black hole. Expand
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