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Table 4:

Best primary candidate calibrators for LOFAR on baselines $\backsim $2 M$\lambda $.
Source Type Redshift RA Dec S327 (Jy)
J0319+4130 (3C 84) Q 0.017559 03h19m48.160s +41d30m42.103s 4.625
J0405+3803 G 0.055000 04h05m49.262s +38d03m32.236s 0.539
J0418+3801 (3C 111) G 0.048500 04h18m21.277s +38d01m35.900s 0.533
J0423-0120 Q 0.914000 04h23m15.801s -01d20m33.065s 1.099
J0539-2839 Q 3.104000 05h39m54.281s -28d39m55.948s 0.564
J1150-0024 Q 1.976200 11h50m43.871s -00d23m54.205s 3.403
J1642+3948 (3C 345) Q 0.592800 16h42m58.810s +39d48m36.994s 3.492
J1816+3457 G 0.244800 18h16m23.901s +34d57m45.748s 0.729
J2005+7752 Q 0.342000 20h05m30.999s +77d52m43.248s 0.602
J2022+6136 G 0.227000 20h22m06.682s +61d36m58.805s 0.990
J2202+4216 (BL Lac) Q 0.068600 22h02m43.291s +42d16m39.980s 1.798
J2253+1608 (3C 454.3) Q 0.859000 22h53m57.748s +16d08m53.561s 8.659
J2327+0940 Q 1.843000 23h27m33.581s +09d40m09.463s 0.396
J2330+1100 Q 1.489000 23h30m40.852s +11d00m18.710s 0.844

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