Time dependence of AGN pair echo, and halo emission as a probe of - - PowerPoint PPT Presentation
Time dependence of AGN pair echo, and halo emission as a probe of extragalactic magnetic fields FO, Murase & Kotera, 2017, in prep FO, Murase & Kotera, PoS(ICRC2017)869 FO, Murase & Kotera, A&A 568, A110 (2014) ICRC2017 Foteini
FO, Murase & Kotera, 2017, in prep FO, Murase & Kotera, PoS(ICRC2017)869 FO, Murase & Kotera, A&A 568, A110 (2014)
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Fermi H.E.S.S.
FO, Murase & Kotera PoS(ICRC2017)869
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108 109 1010 1011 1012 1013 1014
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Fermi H.E.S.S.
108 109 1010 1011 1012 1013 1014
10-2 10-1 100 101 102 103
Fermi H.E.S.S.
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108 109 1010 1011 1012 1013 1014
10-2 10-1 100 101 102 103
Fermi H.E.S.S.
108 109 1010 1011 1012 1013 1014
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Fermi H.E.S.S.
108 109 1010 1011 1012 1013 1014
10-2 10-1 100 101 102 103
∆ T =1000000 yrs
B = 10-16 G, θV =0°
FO, Murase & Kotera PoS(ICRC2017)869
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108 109 1010 1011 1012 1013 1014
10-2 10-1 100 101 102 103
Fermi H.E.S.S.
108 109 1010 1011 1012 1013 1014
10-2 10-1 100 101 102 103
Fermi H.E.S.S.
108 109 1010 1011 1012 1013 1014
10-2 10-1 100 101 102 103
∆ T =1000000 yrs
B = 10-16 G, θV =0°
108 109 1010 1011 1012 1013 1014
10-2 10-1 100 101 102 103
∆ T =1000000 yrs
B = 10-16 G, θV =0° B = 10-15 G, θV =0°
FO, Murase & Kotera PoS(ICRC2017)869
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108 109 1010 1011 1012 1013 1014
10-2 10-1 100 101 102 103
Fermi H.E.S.S.
108 109 1010 1011 1012 1013 1014
10-2 10-1 100 101 102 103
Fermi H.E.S.S.
108 109 1010 1011 1012 1013 1014
10-2 10-1 100 101 102 103
∆ T =1000000 yrs
B = 10-16 G, θV =0°
108 109 1010 1011 1012 1013 1014
10-2 10-1 100 101 102 103
∆ T =1000000 yrs
B = 10-16 G, θV =0° B = 10-15 G, θV =0°
108 109 1010 1011 1012 1013 1014
10-2 10-1 100 101 102 103
∆ T =1000000 yrs
B = 10-16 G, θV =0° B = 10-15 G, θV =0° B = 10-14 G, θV =0°
FO, Murase & Kotera PoS(ICRC2017)869
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108 109 1010 1011 1012 1013 1014
energy/eV
10-2 10-1 100 101 102 103
E2 dN/dE [eV cm-2 s-1]
∆ T =10 yrs
B = 10-18 G, θV =0° B = 10-17 G, θV =0° B = 10-16 G, θV =0°
FO, Murase & Kotera, 2017 [PoS(ICRC2017)869]
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108 109 1010 1011 1012 1013 1014
energy/eV
10-2 10-1 100 101 102 103
E2 dN/dE [eV cm-2 s-1]
∆ T =1000000 yrs
B = 10-16 G, θV =0° B = 10-15 G, θV =0° B = 10-14 G, θV =0°
Neronov & Semikoz 2009
0.1 0.2 0.3 0.4 0.5
θ2 [deg2]
10-2 100 102 104
dN/dθ2 [deg-2]
∆ T =1000000.0 yrs E =10.0-100.0 GeV
B = 10-15.0 G B = 10-16.0 G B = 10-17.0 G
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Neronov & Semikoz 2009
0.1 0.2 0.3 0.4 0.5
θ2 [deg2]
10-2 100 102 104
dN/dθ2 [deg-2]
∆ T =1000000.0 yrs E =10.0-100.0 GeV
B = 10-15.0 G B = 10-16.0 G B = 10-17.0 G
0.1 0.2 0.3 0.4 0.5
θ2 [deg2]
10-2 100 102 104
dN/dθ2 [deg-2]
B = 10-17.0 G E =10.0-100.0 GeV
t =100.0 yrs t =10000.0 yrs t =1000000.0 yrs
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Blumenthal & Gould 1970
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Gabici, Aharonian 2005,7 Kotera, Allard, Lemoine 2011 FO, Murase, Kotera 2014 deabsorbed
Tavecchio 2014
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Gabici, Aharonian 2005,7 Kotera, Allard, Lemoine 2011 FO, Murase, Kotera 2014
0.1 nG
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E [eV] E2 dN/dE [eV s−1 cm−2]
B = 6nG B = 16nG B = 100nG B = 316nG HESS VERITAS Fermi/LAT
Example 1ES 0229+200 (LCR,ISO = 1046.5 erg s -1)
FO, Murase & Kotera, A&A 568, A110 (2014) 9 9
Gabici, Aharonian 2005,7 Kotera, Allard, Lemoine 2011 FO, Murase, Kotera 2014
0.1 nG
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E [eV] E2 dN/dE [eV s−1 cm−2]
B = 6nG B = 16nG B = 100nG B = 316nG HESS VERITAS Fermi/LAT
Example 1ES 0229+200 (LCR,ISO = 1046.5 erg s -1)
FO, Murase & Kotera, A&A 568, A110 (2014) 9 9
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Kotera et al. 2011
D = 1 Gpc B = 1 nG Eγ = 1−100 GeV LCR,19 = 1046 erg s−1 GeV cm−2 s−1
D = 100 Mpc at level of total CR flux
angular extension θ
D = 1 Gpc 10% of total CR flux
Kotera et al. 2011
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Murase 2009,12 Dermer et al.
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FO, Murase & Kotera, 2017 [PoS(ICRC2017)869]
Murase 2009,12 Dermer et al.
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1ES 0229+200 E [eV] E2 dN/dE [eV s−1 cm−2]
UHECR, B =100 nG UHECR, B = 316 nG UHE , B=100 nG UHE , B = 316 nG HESS VERITAS Fermi/LAT
UHE photons B3 Mpc = 316 nG α = 2, Eγ,ΜΑΧ = 1019.5 eV LCR,j ~ 1045 erg s -1
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FO, Murase & Kotera, 2017 [PoS(ICRC2017)869]
Murase 2009,12 Dermer et al.
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1ES 0229+200 E [eV] E2 dN/dE [eV s−1 cm−2]
UHECR, B =100 nG UHECR, B = 316 nG UHE , B=100 nG UHE , B = 316 nG HESS VERITAS Fermi/LAT
UHE photons B3 Mpc = 316 nG α = 2, Eγ,ΜΑΧ = 1019.5 eV LCR,j ~ 1045 erg s -1
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FO, Murase & Kotera, 2017 [PoS(ICRC2017)869]
Murase 2009,12 Dermer et al.
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1ES 0229+200 E [eV] E2 dN/dE [eV s−1 cm−2]
UHECR, B =100 nG UHECR, B = 316 nG UHE , B=100 nG UHE , B = 316 nG HESS VERITAS Fermi/LAT
UHE photons B3 Mpc = 316 nG α = 2, Eγ,ΜΑΧ = 1019.5 eV LCR,j ~ 1045 erg s -1
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FO, Murase & Kotera, 2017 [PoS(ICRC2017)869]
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14 Aharonian et al, Phys.Rev. D87 (2013) no.6, 063002
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Chen et al. Phys.Rev.Lett. 115 (2015)
24 Fermi stacked BL Lacs 0.069 < z < 0.5 Θ = 0.5º Consistent with B = 10-17-10-15 G (if sources steady)
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e.g., Essey et al 2010a,b, Murase et al 2012, Tavecchio 2014
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Takami et al. 2014
e.g., Essey et al 2010a,b, Murase et al 2012, Tavecchio 2014
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Takami et al. 2014
deabsorbed
Tavecchio 2014
e.g., Essey et al 2010a,b, Murase et al 2012, Tavecchio 2014
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Takami et al. 2014
deabsorbed
Tavecchio 2014
e.g., Essey et al 2010a,b, Murase et al 2012, Tavecchio 2014
γ
Kotera et al, 2011
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