#1) Sou: 1219-309 Freq: 9000 Ra: 12_22_14.71 -+ 0.91 Dec: -31_13_35.5 -+ 11.30 Flux: 0.31 -+ 0.04 #2) Sou: 1219-309 Freq: 9000 Ra: 12_22_20.91 -+ 0.43 Dec: -31_18_47.7 -+ 5.70 Flux: 1.01 -+ 0.06 #3) Sou: 1219-309 Freq: 9000 Ra: 12_22_22.16 -+ 0.54 Dec: -31_15_52.7 -+ 7.04 Flux: 0.31 -+ 0.02 #1) Sou: 1219-309 Freq: 5500 Ra: 12_22_14.64 -+ 0.51 Dec: -31_13_32.5 -+ 6.65 Flux: 0.54 -+ 0.03 #2) Sou: 1219-309 Freq: 5500 Ra: 12_22_20.82 -+ 0.27 Dec: -31_18_51.7 -+ 3.54 Flux: 1.27 -+ 0.03 #3) Sou: 1219-309 Freq: 5500 Ra: 12_22_22.13 -+ 1.08 Dec: -31_16_01.9 -+ 13.90 Flux: 0.21 -+ 0.02 #4) Sou: 1219-309 Freq: 5500 Ra: 12_22_14.33 -+ 0.87 Dec: -31_07_58.7 -+ 11.50 Flux: 2.76 -+ 0.22 #5) Sou: 1219-309 Freq: 5500 Ra: 12_22_17.74 -+ 0.53 Dec: -31_21_05.3 -+ 7.02 Flux: 1.33 -+ 0.06 #6) Sou: 1219-309 Freq: 5500 Ra: 12_22_41.42 -+ 0.17 Dec: -31_20_02.9 -+ 1.84 Flux: 8.44 -+ 0.13Source #3 is the closest object to 122222-311525: it is 6.0" off in right ascension and 28" off in declination. It was detected at both bands. It has flux density 0.31 mJy at 5.5 GHz and spectral index -0.79.
NVSS sources within the field of view:
??? C1218M32 295.78 719.77 122212-310802 12 22 12.62 -31 08 02.4 0.20 4.5 8.0 1.1 47.0 < 35.6 -3.6 11.1 10.0 1.77 -19.0 0.91 7.2 #1 C1218M32 294.66 697.61 122214-311334 12 22 14.17 -31 13 34.7 0.70 7.7 3.4 0.6 < 89.9 < 70.5 S* 26 -0.06 1.04 #3? C1218M32 287.79 689.88 122222-311529 12 22 22.30 -31 15 29.6 0.56 10.1 3.5 0.6 <108. < 54.6 -0.13 1.05
#1 Sou: 1219-309 Freq: 9000 Obj: 3 Ra: 12_22_14.63 -+ 0.72 Dec: -31_13_36.1 -+ 0.96 Flux: 0.63 -+ 0.10 #2 Sou: 1219-309 Freq: 9000 Obj: 1 Ra: 12_22_20.83 -+ 0.66 Dec: -31_18_41.7 -+ 1.25 Flux: 0.90 -+ 0.16 #3 Sou: 1219-309 Freq: 9000 Obj: 2 Ra: 12_22_22.20 -+ 0.82 Dec: -31_15_56.5 -+ 1.24 Flux: 0.28 -+ 0.05
Sou: 1219-309 Freq: 5500 Obj: 7 Ra: 12_22_12.95 -+ 1.52 Dec: -31_09_11.9 -+ 2.81 Flux: 0.78 -+ 0.20 Sou: 1219-309 Freq: 5500 Obj: 9 Ra: 12_22_13.00 -+ 1.05 Dec: -31_16_25.6 -+ 1.45 Flux: 0.26 -+ 0.04 #1 Sou: 1219-309 Freq: 5500 Obj: 4 Ra: 12_22_14.74 -+ 0.55 Dec: -31_13_34.9 -+ 0.78 Flux: 0.49 -+ 0.04 Sou: 1219-309 Freq: 5500 Obj: 8 Ra: 12_22_15.94 -+ 1.31 Dec: -31_06_33.6 -+ 3.28 Flux: 5.37 -+ 1.36 Sou: 1219-309 Freq: 5500 Obj: 2 Ra: 12_22_17.64 -+ 0.61 Dec: -31_20_55.3 -+ 1.10 Flux: 1.10 -+ 0.11 Sou: 1219-309 Freq: 5500 Obj: 10 Ra: 12_22_19.24 -+ 1.11 Dec: -31_13_46.0 -+ 1.68 Flux: 0.20 -+ 0.03 #2 Sou: 1219-309 Freq: 5500 Obj: 3 Ra: 12_22_20.84 -+ 0.53 Dec: -31_18_42.9 -+ 0.72 Flux: 0.70 -+ 0.05 Sou: 1219-309 Freq: 5500 Obj: 6 Ra: 12_22_21.87 -+ 1.90 Dec: -31_18_01.6 -+ 2.48 Flux: 0.17 -+ 0.04 #3 Sou: 1219-309 Freq: 5500 Obj: 5 Ra: 12_22_22.25 -+ 0.62 Dec: -31_15_56.3 -+ 0.92 Flux: 0.33 -+ 0.03 Sou: 1219-309 Freq: 5500 Obj: 11 Ra: 12_22_31.69 -+ 1.14 Dec: -31_10_58.6 -+ 1.74 Flux: 0.51 -+ 0.09 Sou: 1219-309 Freq: 5500 Obj: 1 Ra: 12_22_41.39 -+ 0.28 Dec: -31_19_30.3 -+ 0.30 Flux: 5.16 -+ 0.17The closes source to 122222-311525, #3, is in 32.4". The formal uncertainties, 0.6" and 0.9" are a bit too optimistic. More realistic uncertainties will be 1.5-2". But source #3 lies 15-20σ away from source 122222-311525. This is definitely another source.
No source brighter 150 μJy was detected at 5.5 and 9.0 GHz (5σ level) in the vicinity of 122222-311525
Last update: 2013.01.22_10:48:17
Web page was prepared by Leonid Petrov
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