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Table 3.

List of spatiotemporal associations with WT > 0.316 between the updated IceCat1+ neutrinos and blazars of RFC and 4LAC.

CAZ J2000 IC ID MJD 𝒮 Ω WT origin=c]90 RFC origin=c]90 4LAC origin=c]90 BB95 origin=c]90 BBHOP T νsy z Dvar SX-ray
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15)
J0211+1051 131014A 56579.9 0.67 4.5 0.665 Y Y Y* Y* B 14.2 0.2 8.4 5.6e-12
J0207+0950 131014A 56579.9 0.67 4.5 0.665 Y Y Y U 13.4 0.6 1.7e-12
J0509+0541 170922A 58018.9 0.63 4.9 0.631 Y Y Y* Y* B 14.6 0.3 14.7 3.5e-12
J0212−0221 230724A 60149.1 0.53 3.6 0.526 Y Y Y B 14.7 0.2 7.9e-12
J2251+4030 131108A 56604.6 0.50 8.9 0.502 Y Y B 0.2 5.0e-13
J1103+1158 200109A 58858.0 0.77 20.6 0.387 Y Y Y Q 14.1 0.9 1.5e-12
J1615+2130 190413B 58586.7 0.38 8.8 0.383 Y Y U 13.1 1.6
J1619+2247 190413B 58586.7 0.38 8.8 0.383 Y Y Q 2.0 9.4
J2304+2331 100608X 55355.5 0.72 20.2 0.370 Y Y Q 1.2
J1018+1036 220317A 59655.1 0.36 10.6 0.356 Y Y U 0.7
J1819+2132 220822A 59813.9 0.38 11.8 0.335 Y Y B 14.3 0.4 3.3e-13
J1058+1951 130408A 56390.2 0.53 16.4 0.331 Y Y Q 1.1 1.3 2.2e-12
J1117+2014 130408A 56390.2 0.53 16.4 0.331 Y Y B 16.2 0.1 6.8e-12
J1059+2057 130408A 56390.2 0.53 16.4 0.331 Y Y Y Q 0.4 13.6 1.0e-12

Notes. Column (1) gives the CAZ J2000 name of the spatiotemporally associated blazar; (2) IceCube ID of the spatiotemporally associated neutrino; (3) arrival MJD of the neutrino; (4) signalness of the neutrino; (5) area of the enlarged ≳90% error region of the neutrino; (6) top-hat weight of the neutrino; (7) presence of the blazar in the RFC sample; (8) presence of the blazar in the 4LAC sample; (9) temporal association via a BB95 period; (10) temporal association via a prominent BBHOP flare; (11) blazar type from the CAZ catalog; (12) synchrotron peak frequency in log(Hz); (13) redshift; (14) radio variability Doppler factor; and (15) median flux density in the X-ray band (in erg cm−2 s−1). In columns (7)–(10), “Y” means “present”. In columns (9) and (10), “*” indicates an association based on the BB95 as the peak of BBHOP metric (i.e., when the spatially associated neutrino falls within ±2 d of the peak of a prominent BBHOP such that the peak itself is a BB95; see Sect. 2.2.6). For brevity, this table only shows blazar-neutrino spatiotemporal associations with WT > 0.316 (i.e., those with higher than median weight), hiding 96 low-weight associations. The full list of the spatial and spatiotemporal associations is given as an electronic table.

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