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Variability pattern and the spectral evolution of blazars
J. Kataoka
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Physics & Astronomy
blazars
100%
flares
32%
particle accelerators
20%
spectral energy distribution
18%
light curve
16%
x rays
14%
rays
14%
synchrotrons
14%
time lag
13%
cooling
11%
magnetic fields
8%
Earth & Environmental Sciences
magnetic field
24%
cooling
19%
particle
13%
energy
13%
distribution
9%