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Peter BIERMANN (.pdf)

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The radio background, Thomson depth III<br />

Predicted neutrino flux - observed now (IceCube 2013,<br />

lecture by Whitehorn: match!).<br />

Fneutr = 10 −10.2 NBH,0,0 E57 ηCR,p,−1 fneutr,−1 z 0.5<br />

1.3<br />

erg cm −2 s −1 sr −1 , (7)<br />

Mass of shell in gas (Kormendy et al. 2010, 2011)<br />

23<br />

(8)<br />

57 z−3/5<br />

1.3<br />

M shell = 10 10.4 M⊙ E 3/5<br />

Thomson depth through remnant (detected 0.09):<br />

(9)<br />

τT h,Σ = 10 −1.6 NBH,0,0 E 3/5<br />

57 z+9/10<br />

1.3<br />

FIR back ground contribution (matches limit):<br />

FIR = 10 −6.0 erg cm −2 s −1 sr −1 NBH,0,0 MSMS,6.5 z −1<br />

1.3

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