|
astro-ph/9401024 🔍 (source)
|
effective temperature of the high-energy exponential tail |
|
15000000.0 K |
|
|
astro-ph/0104343 🔍 (source)
|
steep high-energy spectral index |
\Gamma |
-2.8 |
|
|
astro-ph/0203181 🔍 (source)
|
flux of upward-going muons from high-energy neutrinos |
|
1.7e-14 cm-2 s-1 sr-1 |
|
|
astro-ph/0607233 🔍 (source)
|
normalization constant of the high-energy neutrino emission |
\gamma |
6.1 TeV-1 m-2 s-1 |
|
|
0708.2002 🔍 (source)
|
high-energy cutoff |
\epsilon _ { c } |
1.2 ± 0.3 keV |
|
|
0811.0983 🔍 (source)
|
high-energy |
E _ { cut } |
16.0 +5.0-3.0 keV |
|
|
1009.1432 🔍 (source)
|
high-energy emission |
t |
2.0 |
Upper |
|
1102.4974 🔍 (source)
|
high-energy |
|
82.0 ± 9.0 keV |
|
|
1207.3308 🔍 (source)
|
high-energy cut-off |
E _ { cut } |
227.0 +143.0-67.0 keV |
|
|
1612.05871 🔍 (source)
|
high-energy cutoff |
E _ { c } |
53.0 +11.0-8.0 keV |
|
|
1805.00480 🔍 (source)
|
consequently fading high-energy radiative emission |
t _ { p } / t _ { A } |
2.0 ± 1.0 |
Upper |
|
1901.04188 🔍 (source)
|
mean high-energy cut-off |
\sigma |
45.0 keV |
|
|
1903.05429 🔍 (source)
|
flux of ultrahigh-energy cosmic rays |
J ( > 10 ^ { 11.3 } ~ { } { GeV } |
3.6e-05 yr km-2 sr-1 %-1 |
Upper |
|
1905.06818 🔍 (source)
|
ratio of the radio to high-energy fluence |
\nicefrac { f _ { r } } f _ { \gamma } |
0.1 |
|