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Table A.1

Expected 0.1−10 PeV flux (in units of 10-8 GeV cm-2 s-1) and detection rate of muon neutrinos Rν (yr-1) for the brightest 2FHL BL Lacs with KM3NeT with different thresholds on the zenith angle (horizon and + 10°).

Name F ν R ν Visibility R ν Visibility
at horizon at 10°
1 Mkn421 8.77 4.59 0.30 5.80 0.39
2 PKS2155-304 2.15 2.23 0.60 2.53 0.69
3 Mkn501 3.41 1.65 0.28 2.26 0.39
4 PG1553+113 1.89 1.42 0.44 1.66 0.51
5 PKS0447-439 0.76 0.87 0.67 1.02 0.79
6 PKS1424+240 1.00 0.67 0.39 0.79 0.46
7 PKS2005-489 0.51 0.63 0.72 0.75 0.86
8 TXS0518+211 0.87 0.59 0.39 0.72 0.48
9 PG1218+304 0.92 0.55 0.34 0.69 0.44
10 1ES0647+250 0.75 0.47 0.36 0.60 0.46
11 3C66A 0.87 0.38 0.25 0.54 0.36
12 1RXSJ054357.3-55320 0.30 0.40 0.78 0.52 1.00
13 PKS0301-243 0.43 0.44 0.59 0.49 0.66
14 1H1914-194 0.45 0.44 0.57 0.49 0.63
15a 1H1013+498 0.87 – – 0.48 0.32
15b 1RXSJ194246.3+10333 0.41 0.32 0.45 – –
16 PKS1440-389 0.36 0.41 0.66 0.47 0.76
17 1ES0347-121 0.39 0.35 0.53 0.40 0.60
18 1ES1215+303 0.52 0.31 0.34 0.39 0.44
19 1RXSJ101015.9-31190 0.32 0.34 0.60 0.39 0.69
20 RXJ0648.7+1516 0.45 0.33 0.42 0.38 0.49

Notes. We also report the fraction of the observational time for which each source is below the threshold. The numbers identify the sources in the sky map, Fig. 3.

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