Fermi LAT observations of cosmic-ray electrons from 7 GeV to 1 TeV

  title={Fermi LAT observations of cosmic-ray electrons from 7 GeV to 1 TeV},
  author={Fermi Lat Collaboration},
M. Ackermann, M. Ajello, W. B. Atwood, L. Baldini, J. Ballet, G. Barbiellini, 6 D. Bastieri, 8 B. M. Baughman, K. Bechtol, F. Bellardi, R. Bellazzini, F. Belli, 11 B. Berenji, R. D. Blandford, E. D. Bloom, J. R. Bogart, E. Bonamente, 13 A. W. Borgland, T. J. Brandt, 9 J. Bregeon, A. Brez, M. Brigida, 16 P. Bruel, R. Buehler, T. H. Burnett, G. Busetto, 8 S. Buson, 8 G. A. Caliandro, R. A. Cameron, P. A. Caraveo, P. Carlson, 22 S. Carrigan, J. M. Casandjian, M. Ceccanti, C. Cecchi, 13 Ö. Çelik… 
Implications of a possible TeV break in the cosmic-ray electron and positron flux
A TeV spectral break in the total flux of cosmic-ray electrons and positrons (CREs) at which the spectral power index softens from $\sim 3$ to $\sim 4$ has been observed by H.E.S.S. and recently
A review of Cosmic-ray electrons and fermi-LAT
The study of Galactic Cosmic-ray electrons (CREs) saw important developments in recent years, with the assumption of positron production only in interaction of hadronic Cosmic-rays with interstellar
Searching for Anisotropies in the Arrival Directions of Electromagnetic Air Showers at TeV energies with H.E.S.S.
The measurements of cosmic-ray electrons and positrons with PAMELA (Adriani et al. 2009), Fermi-LAT (Ackermann et al. 2012) and AMS-02 (Aguilar et al. 2013) have established the existence of an
The energy spectrum of cosmic electrons measured with the MAGIC telescopes
This thesis seeks to further explore the origin of cosmic electrons and positrons. The unexpected excess of very-high-energy electrons above 100 GeV has been established and is now considered proof
Search for gamma-ray emission from supernova remnantswith the Fermi /LAT and MAGIC telescopes
This thesis is an astrophysical approach to the problem of the Galactic cosmic rays. Cosmic rays are energetic particles that hit the Earth atmosphere from above. The discovery of its
P o S ( T e x a s 2 0 1 0 ) 2 1 1 Search for a DM annihilation signal from the Galactic Centre halo with H .
The H.E.S.S. experiment, an array of four Imaging Atmospher ic Cherenkov Telescopes, observes the Galactic Centre (GC) region in the very high-energy (VHE , E > 100 GeV)γ-ray domain since 2003. The
'Discrepant hardenings' in cosmic ray spectra: A first estimate of the effects on secondary antiproton and diffuse gamma-ray yields
Recent data from CREAM seem to confirm early suggestions that primary cosmic ray spectra at few TeV/nucleon are harder than in the 10-100 GeV range. Also, helium and heavier nuclei spectra appear
D ec 2 01 2 Gamma Ray Signals from Dark Matter : Concepts , Status and Prospects
Weakly interacting massive particles (WIMPs) remain a prim e candidate for the cosmological dark matter (DM), even in the absence of current co llider signals that would unambiguously point to new


Annual Review Of Nuclear And Particle Science
The contents of this review reflect some of the shifts of emphasis that are occurring among the fields of astrophysics, nuclear physics, and elementary particle physics. Particle physics has made
however (for it was the literal soul of the life of the Redeemer, John xv. io), is the peculiar token of fellowship with the Redeemer. That love to God (what is meant here is not God’s love to men)
北京大学濮祖荫教授被推选为国际著名期刊Journal of Geophysical Research——Space Physics的主编
北京大学地球与空间科学学院濮祖荫教授被美国地球物理学会任命为Journal of Geophysical Research(Space Physics)的新一届亚洲与太平洋区域主编,任期为4年(2006-2009).
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