Table 1
List of Fermi sources for which a 100 GeV ≤ E ≤ 300 GeV photon is found within the 68% containment circle of radius 0.1°.
1FGL | RA | Dec | N68 | P68 | N68 | Nmin | P | TS | Type1 | Name | z | ||
30−100 | 30−100 | 100−300 | [N95] | 100−300 | |||||||||
|
|||||||||||||
1 | J0033.5-1921 | 8.3913 | –19.3650 | 6 | 2.1 × 10-14 | 1b | 1 | 2.3 × 10-5 | 21 | BL V | RBS 76 | 0.61 | |
2 | J0054.9-2455 | 13.7337 | –24.9290 | 0 | – | 1f | 3.2 × 10-3 | 18 | |||||
3 | J0110.0-4023 | 17.5250 | –40.3887 | 1 | 1.3 × 10-2 | 1f | 2.4 × 10-3 | 12 | |||||
4 | J0209.3-5229 | 32.3392 | –52.4907 | 2 | 1.1 × 10-4 | 1f | 3.5 × 10-3 | 12 | BL Vf | RBS 285 | |||
5 | J0213.2+2244 | 33.3225 | 22.7489 | 2 | 1.6 × 10-4 | 1b | 2.6 × 10-3 | 13 | QSO | 1RXS | |||
J021252.2+22 | |||||||||||||
6 | J0222.6+4302 | 35.6681 | 43.0385 | 16 | 4.6 × 10-40 | 3f1b | 1 | 1.4 × 10-13 | 75 | BL V | 3C 66A | 0.444 | |
7 | J0237.5-3603 | 39.3788 | –36.0530 | 3 | 2.3 × 10-7 | 1b | 2.4 × 10-3 | 15 | BL V | RBS 334 | |||
8 | J0303.5-2406 | 45.8890 | –24.1124 | 9 | 2.0 × 10-23 | 2f | [1] | 1.8 × 10-6 | 39 | BL Vf | PKS 0301-243 | 0.26 | |
9 | J0315.9-2609 | 48.9933 | –26.1581 | 1 | 1.4 × 10-2 | 2b | 3.5 × 10-6 | 28 | BL V | RX J0316.2-2607 | 0.443 | ||
10 | J0316.3-6438 | 49.0996 | –64.6411 | 0 | – | 1b | 1.5 × 10-3 | 13 | |||||
11 | J0322.1+2336 | 50.5396 | 23.6108 | 2 | 2.0 × 10-4 | 1f | 4 × 10-3 | 16 | BL Vf | RGB J0321+236 | |||
12 | J0325.9-1649 | 51.4780 | –16.8174 | 0 | – | 1b | 2.5 × 10-3 | 12 | BL V | RBS 421 | 0.29 | ||
13 | J0338.8+1313 | 54.7212 | 13.2314 | 0 | – | 1b | 3.1 × 10-3 | 13 | |||||
14 | J0416.8+0107 | 64.2069 | 1.1244 | 0 | – | 1f | 2.5 × 10-3 | 14 | BL Vf | 2E 0414+0057 | |||
15 | J0428.6-3756 | 67.1567 | –37.9412 | 9 | 3.4 × 10-22 | 1f | 2.9 × 10-3 | 18 | BL | PKS 0426-380 | 1.11 | ||
16 | J0505.9+6121 | 76.4853 | 61.3527 | 1 | 1.9 × 10-2 | 1f | [2] | 1.6 × 10-6 | 21 | ||||
17 | J0507.9+6738 | 76.9931 | 67.6367 | 12 | 2.7 × 10-29 | 2f2b | 3 | 3.8 × 10-19 | 96 | BL V | 1ES 0502+675 | 0.341 | |
18 | J0543.8-5531 | 85.9512 | –55.5301 | 1 | 2.0 × 10-2 | 1f1b | 5.3 × 10-6 | 34 | BL V | RBS 679 | |||
19 | J0650.7+2503 | 102.6817 | 25.0622 | 1 | 1.0 × 10-2 | 1f | 2.2 × 10-3 | 15 | BL V | 1ES 0647+250 | 0.203 | ||
20 | J0710.6+5911 | 107.6595 | 59.1853 | 3 | 2.3 × 10-6 | 1f | 2.0 × 10-3 | 17 | BL | RX J0710.4+5908 | 0.125 | ||
21 | J0721.9+7120 | 110.4794 | 71.3448 | 9 | 6.3 × 10-21 | 1f | 3.6 × 10-3 | 13 | BL Vf | S5 0716+71 | 0.3 | ||
22 | J0745.2+7438 | 116.3215 | 74.6415 | 0 | – | 1b | 3.9 × 10-3 | 10 | BL V | 1ES 0737+746 | 0.315 | ||
23 | J0809.4+3455 | 122.3539 | 34.9331 | 0 | – | 1f | 2.5 × 10-3 | 14 | BL Vf | B2 0806+35 | 0.0825 | ||
24 | J0809.5+5219 | 122.3856 | 52.3178 | 5 | 3.1 × 10-11 | 1f1b | 5.9 × 10-6 | 25 | BL Vf | 1ES 0806+524 | 0.138 | ||
25 | J0816.4-1311 | 124.1121 | –13.1933 | 5 | 5.5 × 10-13 | 1f | 1.8 × 10-3 | 13 | BL Vf | PMN J0816-1311 | |||
26 | J0905.5+1356 | 136.3916 | 13.9483 | 1 | 1.5 × 10-2 | 1b | 4.0 × 10-3 | 14 | QSO? | SDSS J090513.28 | 1.12 | ||
+140240.3 | |||||||||||||
27 | J0915.7+2931 | 138.9412 | 29.5319 | 3 | 8.6 × 10-7 | 1f | 2.7 × 10-3 | 13 | BL Vf | B2 0912+29 | |||
28 | J0953.0-0838 | 148.2673 | –8.6461 | 2 | 9.5 × 10-5 | 1f | 2.6 × 10-3 | 15 | BL Vf | PMN J0953-840 | |||
29 | J0957.7+5523 | 149.4315 | 55.3922 | 6 | 2.1 × 10-13 | 1b | 3.6 × 10-3 | 12 | QSO | 4C +55.17 | 0.8955 | ||
30 | J1015.1+4927 | 153.7885 | 49.4526 | 5 | 2.9 × 10-11 | 1b | 2 | 2.6 × 10-7 | 35 | BL V | 1ES 1011+496 | 0.212 | |
31 | J1104.4+3812 | 166.1247 | 38.2108 | 57 | 0 | 14f8b | 3[1] | 0 | 494 | BL V | Mkn 421 | 0.03 | |
32 | J1117.1+2013 | 169.2993 | 20.2222 | 3 | 5.5 × 10-7 | 1f | 2.9 × 10-3 | 12 | BL Vf | RBS 958 | 0.1 | ||
33 | J1133.1+0033 | 173.2792 | 0.56306 | 0 | – | 1f | 2.9 × 10-3 | 11 | BL V | PKS B1130+008 | 1.223 | ||
34 | J1217.7+3007 | 184.4463 | 30.1206 | 2 | 2.0 × 10-4 | 1b | 3.0 × 10-3 | 8 | BL V | B2 1215+30 | 0.13 | ||
35 | J1224.7+2121 | 186.1987 | 21.3633 | 6 | 7.3 × 10-14 | 1f1b | 1.7 × 10-6 | 31 | FSRQ | 4C +21.35 | 0.432 | ||
36 | J1309.5+4304 | 197.3933 | 43.0669 | 3 | 8.8 × 10-7 | 1f | 2.9 × 10-3 | 13 | BL Vf | B3 1307+433 | 0.69 | ||
37 | J1337.7-1255 | 204.4336 | –12.9289 | 0 | – | 1f | 1.5 × 10-3 | 15 | FSRQ | PKS 1335-127 | 0.539 | ||
38 | J1437.0+5640 | 219.2617 | 56.6720 | 4 | 5.7 × 10-9 | 1f | 3.4 × 10-3 | 17 | BL | RBS 1409 | 0.15 | ||
39 | J1555.7+1111 | 238.9383 | 11.1921 | 25 | 0 | 3f2b | 1[1] | 3 × 10-16 | 124 | BL V | PG 1553+113 | ||
40 | J1653.9+3945 | 253.4897 | 39.7527 | 17 | 1.1 × 10-44 | 9f1b | 1 | 1.5 × 10-32 | 214 | BL V | Mkn 501 | 0.0336 | |
41 | J1722.5+1012 | 260.6494 | 10.2144 | 0 | – | 1f | 2.3 × 10-3 | 17 | FSRQ | TXS 1720+102 | |||
42 | J1744.2+1934 | 266.0710 | 19.5706 | 1 | 2.1 × 10-2 | 1b | 2.5 × 10-3 | 13 | BL V | 1ES 1741+196 | 0.083 | ||
43 | J1824.6+1013 | 276.1739 | 10.2180 | 0 | – | 1f | 1.9 × 10-3 | 10 | |||||
44 | J2000.0+6508 | 300.0215 | 65.1334 | 7 | 2.1 × 10-15 | 1f | [1] | 1.9 × 10-4 | 20 | BL Vf | 1ES 1959+650 | 0.048 | |
45 | J2000.9-1749 | 300.2467 | –17.8286 | 1 | 2.2 × 10-2 | 1b | 4.0 × 10-3 | 11 | FSRQ | PKS 1958-179 | 0.65 | ||
46 | J2004.8+7004 | 301.2074 | 70.0710 | 0 | – | 1b | 4.3 × 10-3 | 13 | |||||
47 | J2009.5-4849 | 302.3761 | –48.8295 | 7 | 1.3 × 10-15 | 4f1b | [1] | 7.5 × 10-15 | 82 | BL V | PKS 2005-489 | 0.071 | |
48 | J2158.8-3013 | 329.7117 | –30.2176 | 23 | 0 | 5f3b | 1[1] | 2.2 × 10-24 | 164 | BL V | PKS 2155-304 | 0.117 | |
49 | J2314.1+1444 | 348.5487 | 14.7463 | 1 | 1.8 × 10-2 | 1f | 3.1 × 10-3 | 13 | AGN | SDSS J231405.46 | 1.319 | ||
+143904.6 | |||||||||||||
50 | J2322.6+3435 | 350.6540 | 34.5839 | 1 | 2.0 × 10-2 | 1f | 3.4 × 10-3 | 14 | BL | TXS 2320+343 | 0.098 |
Notes. First column: Fermi source ID; 2nd column: Right Accention; 3rd column: Declination; 4th column: number of photons in the 68% containment circle in 30 − 100 GeV band; 5th column: chance coincidence probability to find given number of photons in the 68% containment circle in 30−100 GeV band; 6th column: number of photons in the 68% containment circle in 100−300 GeV band; “f” marks front photons, “b” marks back photons; 7th column: number of photons in the θ ≤ 0.17° circle around the source or in the 95% containment circle of the radius 0.3° (square brackets); 8th column: chance probability to find given number of background photons within 0.1° and 0.17° [0.3°] circles around the source position; 9th column: TS value in 100−300 GeV energy bin, found with our analysis; 10th column: source type; 11th column: alternative name of the source; 12th column: source redshift. Bold marks the sources which have been previously detected in the VHE band by ground-based γ-ray telescopes. Underlined are sources detected with Fermi in 100 − 300 GeV band with TS > 25. The updated version of this table is available online at http://www.isdc.unige.ch/vhe/.1 BL – BL Lac type object; QSO – quasi-stellar object, AGN – active galactic nucleus, FSRQ – flat spectrum radio quasar; FR I – Fanaroff-Riley type I radio galaxy; V – also found from the correlation analysis with the BL Lac catalog; Vf – front photon contributes to the correlation signal with the BL Lac catalog.
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