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Table 5

DXRBS sources possibly associated to Fermi objects.

Name FIRST Name 2FGL O.I 2FGL RA 2FGL Dec Radio-γ Sep. Association γ-var. Radio-Var.
NVSS rms [arcmin] rms [arcmin] [arcmin]

J0204.8+1514 J0205.0+1514 SSRQ 8.1 6.5 2.7 4C15.05 T yes
J0510.0+1800 J0509.9+1802 FSRQ 6.5 5.1 1.7 PKS 0507+17 T no
J0847.2+1133 J0847.2+1134 BL Lac 5.3 4.6 0.8 RX J0847.1+1133 no
J0937.1+5008 J0937.6+5009 FSRQ 8.6 2.3 7.4 GB6 J0937+5008 T yes
J1010.80201 J1010.80158 FSRQ 8.3 7.7 4.1 PKS 100801 yes
J1204.20710 J1204.30711 BL Lac 8.0 6.9 1.8 1RXS J120417.0070959 no
J1231.7+2848 J1231.7+2848 BL Lac 2.3 2.2 0.4 B2 1229+29 T no
J1332.7+4722 J1332.7+4725 FSRQ 13.6 13.1 10.4 B3 1330+476 T yes
J1656.8+6012 J1656.5+6012 FSRQ 8.4 7.7 4.5 87GB 165604.4+601702 yes

Name ATCA

J0448.22110 J0448.62118 FSRQ 14.8 10.3 9.9 PKS 0446212
J0449.44349 J0449.44350 BL Lac 1.2 1.1 1.1 PKS 0447439 T
J1610.33958 J1610.64002 FSRQ 18.5 11.5 6.1 PMN J16103958
J1936.84719 J1936.84721 BL Lac 4.1 8.5 2.0 PMN J19364719
J2258.35525 J2258.85524 BL Lac 10.2 9.0 9.1 PMN 22585526
J2330.63724 J2330.63723 BL Lac 7.1 6.5 0.5 PKS 2327376

Notes. Column 1: FIRST, NVSS or ATCA source name; 2: 2FLG source name; 3: optical Identification; 4: right ascention rms from the 2FGL in arcmin; 5: declination rms from the 2FGL in arcmin; 6: separation beetween FIRST, NVSS or ATCA object to 2FGL object in arcmin; 7: name of the associated radio source as suggested in 2FGL; 8: variability as in 2FGL: T indicates <1% chance of being a steady source; 9: radio variability as in Mantovani et al. (2011).

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