Details of the Compton thick sources found in this sample. Column (1): galaxy name; column (2): the directly measured NH (cm−2); column (3): the EW of the Fe Kα line (eV); column (4): the reflection fraction determined from the pexmon model.
| Name | log10(NH) | EW | R |
| (1) | (2) | (3) | (4) |
| NGC 1068 | – | 677 | 10.3 |
| NGC 1320 | 24.3+1.2−0.3 | 940+851−585 | 40.4+44.9−39 |
| NGC 1386 | 20.7+0.1−0.1 | 1710+373−373 | 145+160−147 |
| NGC 1667 | 24.4+1.8−1.1 | – | – |
| NGC 3079 | 20.7+0.3−0.7 | 716+2180−525 | 16.3+7.84−9.7 |
| NGC 3690 | 20.8+0.3−0.8 | 913+380−346 | – |
| MESSIER 088 | 21.3+0.4−0.2 | – | 17.6+24.2−17.6 |
| NGC 4968 | 24.5+0.9−0.3 | 4510+1700−1700 | – |
| NGC 5194 | 20.6+0.1−0.1 | 646+2930−525 | 51.3+31.6−41.1 |
| 2MASX J15504152 | 21.6+0.4−0.7 | – | 13.7+59.5−8.87 |
| NGC 6552 | – | 1490+510−510 | 112+83.2−47.7 |
| NGC 6890 | 21.0+0.5−0.7 | – | 52.1+43.2−47 |
| NGC 7479 | 24.3+0.5−0.4 | 768+429−429 | 0.29+3.71−0.3 |
| ESO 148-IG002 | – | – | 41.6+32.6−43.1 |
| NGC 7582 | 20.6 | 639+197−414 | 107 |
| NGC 7674 | – | 272+173−173 | 143+120−148 |
| Name | log10(NH) | EW | R |
| (1) | (2) | (3) | (4) |
| NGC 1068 | – | 677 | 10.3 |
| NGC 1320 | 24.3+1.2−0.3 | 940+851−585 | 40.4+44.9−39 |
| NGC 1386 | 20.7+0.1−0.1 | 1710+373−373 | 145+160−147 |
| NGC 1667 | 24.4+1.8−1.1 | – | – |
| NGC 3079 | 20.7+0.3−0.7 | 716+2180−525 | 16.3+7.84−9.7 |
| NGC 3690 | 20.8+0.3−0.8 | 913+380−346 | – |
| MESSIER 088 | 21.3+0.4−0.2 | – | 17.6+24.2−17.6 |
| NGC 4968 | 24.5+0.9−0.3 | 4510+1700−1700 | – |
| NGC 5194 | 20.6+0.1−0.1 | 646+2930−525 | 51.3+31.6−41.1 |
| 2MASX J15504152 | 21.6+0.4−0.7 | – | 13.7+59.5−8.87 |
| NGC 6552 | – | 1490+510−510 | 112+83.2−47.7 |
| NGC 6890 | 21.0+0.5−0.7 | – | 52.1+43.2−47 |
| NGC 7479 | 24.3+0.5−0.4 | 768+429−429 | 0.29+3.71−0.3 |
| ESO 148-IG002 | – | – | 41.6+32.6−43.1 |
| NGC 7582 | 20.6 | 639+197−414 | 107 |
| NGC 7674 | – | 272+173−173 | 143+120−148 |
Details of the Compton thick sources found in this sample. Column (1): galaxy name; column (2): the directly measured NH (cm−2); column (3): the EW of the Fe Kα line (eV); column (4): the reflection fraction determined from the pexmon model.
| Name | log10(NH) | EW | R |
| (1) | (2) | (3) | (4) |
| NGC 1068 | – | 677 | 10.3 |
| NGC 1320 | 24.3+1.2−0.3 | 940+851−585 | 40.4+44.9−39 |
| NGC 1386 | 20.7+0.1−0.1 | 1710+373−373 | 145+160−147 |
| NGC 1667 | 24.4+1.8−1.1 | – | – |
| NGC 3079 | 20.7+0.3−0.7 | 716+2180−525 | 16.3+7.84−9.7 |
| NGC 3690 | 20.8+0.3−0.8 | 913+380−346 | – |
| MESSIER 088 | 21.3+0.4−0.2 | – | 17.6+24.2−17.6 |
| NGC 4968 | 24.5+0.9−0.3 | 4510+1700−1700 | – |
| NGC 5194 | 20.6+0.1−0.1 | 646+2930−525 | 51.3+31.6−41.1 |
| 2MASX J15504152 | 21.6+0.4−0.7 | – | 13.7+59.5−8.87 |
| NGC 6552 | – | 1490+510−510 | 112+83.2−47.7 |
| NGC 6890 | 21.0+0.5−0.7 | – | 52.1+43.2−47 |
| NGC 7479 | 24.3+0.5−0.4 | 768+429−429 | 0.29+3.71−0.3 |
| ESO 148-IG002 | – | – | 41.6+32.6−43.1 |
| NGC 7582 | 20.6 | 639+197−414 | 107 |
| NGC 7674 | – | 272+173−173 | 143+120−148 |
| Name | log10(NH) | EW | R |
| (1) | (2) | (3) | (4) |
| NGC 1068 | – | 677 | 10.3 |
| NGC 1320 | 24.3+1.2−0.3 | 940+851−585 | 40.4+44.9−39 |
| NGC 1386 | 20.7+0.1−0.1 | 1710+373−373 | 145+160−147 |
| NGC 1667 | 24.4+1.8−1.1 | – | – |
| NGC 3079 | 20.7+0.3−0.7 | 716+2180−525 | 16.3+7.84−9.7 |
| NGC 3690 | 20.8+0.3−0.8 | 913+380−346 | – |
| MESSIER 088 | 21.3+0.4−0.2 | – | 17.6+24.2−17.6 |
| NGC 4968 | 24.5+0.9−0.3 | 4510+1700−1700 | – |
| NGC 5194 | 20.6+0.1−0.1 | 646+2930−525 | 51.3+31.6−41.1 |
| 2MASX J15504152 | 21.6+0.4−0.7 | – | 13.7+59.5−8.87 |
| NGC 6552 | – | 1490+510−510 | 112+83.2−47.7 |
| NGC 6890 | 21.0+0.5−0.7 | – | 52.1+43.2−47 |
| NGC 7479 | 24.3+0.5−0.4 | 768+429−429 | 0.29+3.71−0.3 |
| ESO 148-IG002 | – | – | 41.6+32.6−43.1 |
| NGC 7582 | 20.6 | 639+197−414 | 107 |
| NGC 7674 | – | 272+173−173 | 143+120−148 |
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