The Spectra of IceCube Neutrino (SIN) candidate sources - V. Modeling and interpretation of multiwavelength and neutrino data

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Table E.1.

Predicted muon neutrino flux, neutrino peak energy, and best-fit parameter values of the leptohadronic model for the blazars in the sample.

Associated source	log₁₀(F_{μ_ν})	E_ν/PeV	log₁₀( $R_{b}^{'}$ $R_{\rm b}^\prime$ )	B′	Γ_b	R_diss/R_BLR	${log}_{10} (γ_{e}^{' \max})$ $\log_{10}(\gamma_{\mathrm{e}}^{\prime\mathrm{max}})$	${log}_{10} (γ_{p}^{' \max})$ $\log_{10}(\gamma_{\mathrm{p}}^{ \prime\mathrm{max}})$	p_e	p_p	log₁₀( $L_{e}^{'}$ $L^\prime_{\rm e}$ )	log₁₀( $L_{p}^{'}$ $L^\prime_{\rm p}$ )	$χ_{r}^{2^{‡}}$ $\chi_{\rm r}^{2^\ddagger}$
TXS 0506+056^*	-10.8	120.1	16.4	1.6	14.8	2.0	4.0	8.1	1.3	1.0	41.9	44.6	99.4
3HSP J111706.2+20140^*	-11.3	5.3	16.4	3.2	4.1	1.6	4.9	7.2	1.3	1.4	42.6	45.9	65.6
3HSP J203057.1+19361^*	-11.5	71.7	15.8	0.8	24.5	1.6	4.4	8.1	1.6	0.9	40.0	43.3	38.4
VOU J150720-370902^*	-11.6	9.9	16.2	8.1	4.6	1.0	4.0	7.9	1.6	1.4	42.3	44.6	110.5
3HSP J064933.6-31392	-11.6	8.8	16.3	2.3	18.6	1.9	5.2	7.3	1.3	1.5	41.2	44.8	111.8
5BZB J2227+0037^*	-11.7	44.7	16.5	0.2	31.6	2.7	4.1	7.9	2.1	1.7	41.3	45.0	92.8
5BZB J1314+2348^*	-11.7	37.8	15.8	1.9	23.4	1.8	3.7	8.2	1.7	1.7	40.9	44.0	44.0
3HSP J034424.9+34301	-11.7	47.2	16.0	1.3	14.8	1.8	4.1	7.9	1.6	1.0	40.0	44.0	244.6
3HSP J153311.2+18542	-11.8	6.2	15.8	3.1	9.1	1.7	5.4	6.9	1.4	1.1	41.5	45.2	33.6
3HSP J155424.1+20112	-11.9	4.4	16.1	6.3	4.1	1.6	5.3	7.2	1.2	1.3	42.5	45.6	38.3
3HSP J094620.2+01045^†	-12.0	3.7	15.2	10.0	14.5	–	5.2	6.7	1.4	1.4	41.2	45.4	60.5
3HSP J095507.9+35510^†	-12.0	46.6	16.1	0.2	24.5	–	6.7	7.5	1.9	1.0	40.8	45.2	54.1
3HSP J023248.5+20171^†	-12.0	110.9	15.7	0.1	31.6	–	6.5	7.8	2.2	1.6	40.3	44.4	57.6
3HSP J100326.6+02045	-12.1	9.4	16.3	3.2	28.2	2.1	4.0	7.2	1.5	2.0	39.4	44.1	91.6
3HSP J213314.3+25285	-12.1	12.4	16.1	0.6	14.8	2.3	4.0	7.2	1.8	1.6	40.7	45.1	57.9
3HSP J152835.7+20042^*	-12.1	11.9	15.2	3.2	16.2	1.6	5.8	7.0	1.6	1.0	40.5	44.6	18.1
3HSP J062753.3-15195^†	-12.1	3.9	15.7	4.7	5.1	–	5.2	7.1	1.4	1.5	42.6	45.2	141.8
CRATESJ180812+350104^*	-12.2	23.3	16.3	1.4	9.1	1.7	4.1	7.8	1.4	1.6	41.7	44.3	24.0
VOU J105603-180929	-12.3	41.5	16.6	1.0	31.6	2.1	4.1	7.7	1.7	1.1	39.6	42.9	64.3
3HSP J085410.1+27542^†	-12.3	172.9	15.6	0.0	35.5	–	4.8	7.9	1.3	1.2	40.5	45.1	57.2
5BZB J1322+3216^*	-12.5	25.9	15.7	4.9	6.5	1.6	4.5	7.9	1.6	1.3	42.6	44.6	29.9
3HSP J203031.6+22343	-12.5	17.3	15.9	0.4	14.5	2.8	5.0	7.3	1.9	1.2	41.1	45.2	116.4
3HSP J222329.5+01022	-12.5	11.1	15.9	0.8	31.6	2.5	4.7	6.9	2.4	1.2	40.4	44.2	208.3
VOU J022411+161500	-12.5	5.7	16.3	0.5	6.5	1.7	3.8	7.3	1.2	1.3	42.3	45.5	48.9
CRATESJ232625+011147^*	-12.5	45.9	16.2	1.1	11.0	2.4	4.6	8.1	1.9	1.4	42.6	45.1	76.5
5BZU J0158+0101^*	-12.6	15.2	16.6	0.8	5.0	1.4	3.9	8.1	2.0	1.6	42.8	44.5	59.5
CRATESJ024445+132002	-12.6	40.4	16.3	4.3	24.5	1.4	6.3	8.5	2.4	1.5	40.8	42.2	61.7
3HSP J023927.2+13273	-12.7	16.1	15.1	3.4	18.6	1.3	3.9	8.3	1.6	2.0	40.6	43.9	45.0
3HSP J180849.7+35204^†	-12.7	57.6	15.0	0.7	24.5	–	4.2	7.3	2.4	1.1	39.9	44.6	126.2
3HSP J112405.3+20455	-12.8	2.9	15.4	7.1	18.6	1.3	4.2	6.4	1.6	1.5	40.7	43.6	191.0
3HSP J112503.6+21430	-12.8	6.4	16.3	0.9	8.5	1.9	5.7	7.5	2.0	2.0	42.1	45.8	66.8
3HSP J125848.0-04474^†	-12.8	18.1	16.3	0.2	15.8	–	6.0	7.2	2.0	1.2	41.4	44.9	43.5
3HSP J130008.5+17553	-12.8	20.6	15.4	5.8	5.0	1.4	4.3	7.9	1.6	1.4	42.7	44.4	44.3
3HSP J125821.5+21235	-13.6	2.1	15.4	4.7	18.6	1.2	4.7	6.0	1.3	1.0	40.1	42.6	84.5

Sample mean	-12.2	16.2	15.9	2.6	16.8	1.8	4.7	7.5	1.7	1.4	41.2	44.5	-
Sample spread (max-min)	2.7	1.9	1.6	10.0	31.4	1.7	3.0	2.5	1.2	1.1	3.4	3.7	-
Average model uncertainty	0.4	< 0.1	0.2	0.2	0.3	0.1	0.3	< 0.1	< 0.1	0.1	0.1	0.3	-

Note: All variables are given in CGS units, except the predicted neutrino peak energy, given in petaelectronvolt. ^‡ Reduced chi-squared value, assuming a number of degrees of freedom of N − 10, where N is the number of data points in the multiwavelength SED and 10 is the number of model parameters. This value does not directly represent the goodness of fit of the model because it includes the effect of the intrinsic variability of the data. As noted in Section 2.4, we do not directly use the chi-squared value to optimize the model, but the derived quantity $χ_{log}^{2}$ $\chi^2_{\rm log}$ , defined in Eq. (2). ^* Source previously identified as a masquerading BL Lac object (cf. Table 1). ^† Source previously identified as a true BL Lac object.

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