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Table 4.
Refined sample of XBCs and outliers that are with high confidence likely BL Lac sources.
| Name 3FGL | Name XRT | Ang. sep. | Class |
|---|---|---|---|
| 3FGLJ0031.6+0938 | SWXRTJ003159.7+093617 | 5.20 | XBC |
| 3FGLJ0430.1−3103 | SWXRTJ042958.8−305935 | 4.99 | XBC |
| 3FGLJ0516.6+1012 | SWXRTJ051641.5+101244 | 0.39 | XBC |
| 3FGLJ0802.3−0941 | SWXRTJ080216.0−094210 | 1.44 | XBC |
| 3FGLJ1117.7+0217 | SWXRTJ111731.0+021555 | 3.76 | XBC |
| 3FGLJ1119.8−2647 | SWXRTJ111957.1−264320 | 4.20 | XBC |
| 3FGLJ1120.6+0713 | SWXRTJ112042.5+071313 | 0.35 | XBC |
| 3FGLJ1200.9−1432 | SWXRTJ120055.0−143041 | 1.85 | XBC |
| 3FGLJ1225.4−3448 | SWXRTJ122536.8−344722 | 2.54 | XBC |
| 3FGLJ1228.4−0317 | SWXRTJ122819.5−031813 | 1.87 | XBC |
| 3FGLJ1249.5−0546 | SWXRTJ124919.6−054539 | 3.17 | XBC |
| 3FGLJ1309.0+0347 | SWXRTJ130832.3+034410 | 8.07 | XBC |
| 3FGLJ1513.3−3719 | SWXRTJ151318.7−372009 | 1.03 | XBC |
| 3FGLJ1810.7+5335 | SWXRTJ181037.9+533502 | 0.95 | XBC |
| 3FGLJ1934.2+6002 | SWXRTJ193419.8+600141 | 1.20 | XBC |
| 3FGLJ2043.6+0001 | SWXRTJ204342.3+000119 | 1.53 | XBC |
| 3FGLJ2044.0+1035 | SWXRTJ204351.6+103406 | 2.46 | XBC |
| 3FGLJ2047.9−3119 | SWXRTJ204806.1−312015 | 2.29 | XBC |
| 3FGLJ2142.7+1957 | SWXRTJ214247.4+195812 | 1.16 | XBC |
| 3FGLJ0216.0+0300 | SWXRTJ021541.3+030431 | 6.51 | OUT |
| 3FGLJ0536.4−3347 | SWXRTJ053629.2−334302 | 4.37 | OUT |
| 3FGLJ0609.7−1841 | SWXRTJ061000.4−183754 | 5.67 | OUT |
| 3FGLJ0737.8−8245 | SWXRTJ073706.5−824841 | 3.33 | OUT |
| 3FGLJ0919.4+6604 | SWXRTJ091913.0+655639 | 8.03 | OUT |
| 3FGLJ0921.6+2339 | SWXRTJ092145.4+233550 | 3.74 | OUT |
| 3FGLJ0941.0+6151 | SWXRTJ094151.4+615100 | 5.45 | OUT |
| 3FGLJ1200.4+0202 | SWXRTJ120056.1+020803 | 9.23 | OUT |
| 3FGLJ1611.9+1404 | SWXRTJ161137.0+141051 | 7.56 | OUT |
| 3FGLJ1809.0+3517 | SWXRTJ180914.8+350903 | 8.29 | OUT |
| 3FGLJ2112.5−3044 | SWXRTJ211211.8−304541 | 5.18 | OUT |
Notes. In Col. 1 we report the 3FGL name, in Col. 2 the Swift/XRT source designation, in Col. 3 the angular separation between the 3FGL and XRT positions, and in Col. 4 the source class.
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