Cosmic-ray electron-positron spectrum from 7 GeV to 2 TeV with the Fermi Large Area Telescope
Apr 21, 201716 pages
Published in:
- Phys.Rev.D 95 (2017) 8, 082007
- Published: Apr 21, 2017
e-Print:
- 1704.07195 [astro-ph.HE]
Report number:
- FERMILAB-PUB-17-188-AE
Experiments:
Citations per year
Abstract: (APS)
We present a measurement of the cosmic-ray electron+positron spectrum between 7 GeV and 2 TeV performed with almost seven years of data collected with the Fermi Large Area Telescope. We find that the spectrum is well fit by a broken power law with a break energy at about 50 GeV. Above 50 GeV, the spectrum is well described by a single power law with a spectral index of 3.07±0.02(stat+syst)±0.04(energy measurement). An exponential cutoff lower than 1.8 TeV is excluded at 95% CL.- 98.70.Sa
- 96.50.sb
- 95.85.Ry
- 95.55.Vj
- positron: spectrum
- electron: cosmic radiation
- electron positron
- GLAST
- power spectrum
References(40)
Figures(27)
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- [6]
- [7]
- [8]
- [9]
- [10]
- [11]
- [12]
- [13]
- [13]
- [14]
- [15]
- [16]
- [17]
- [18]
- [19]
- [20]
- [21]
- [22]
- [23]
- [24]