Table 1
Results of the Monte Carlo Simulations for PAO UHECRs and the BS-A GMF Model.
| Event | l | b | Energy | H | He | O | Al | Ca | Fe | |||||||||||||
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| dist | rms | match | dist | rms | match | dist | rms | match | dist | rms | match | dist | rms | match | dist | rms | match | |||||
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| 0 | 15.4 | 8.4 | 70.0 | 28.0 | 4.9 | – | 118.1 | 73.3 | – | 94.4 | 16.2 | – | 123.9 | 55.8 | – | 119.5 | 62.6 | N 4760 (7) | 121.2 | 57.0 | N 3557 (4) | |
| 1 | –50.8 | 27.6 | 84.0 | 2.7 | 1.4 | – | 5.2 | 2.7 | – | 18.1 | 7.4 | – | 19.1 | 15.9 | N 3557 (7) | 26.4 | 32.0 | I 4296 (6) | 49.7 | 69.1 | I 4296 (12) | |
| 2 | –49.6 | 1.7 | 66.0 | 6.7 | 4.3 | – | 9.0 | 8.5 | N 5128 (5) | 15.4 | 30.3 | – | 60.5 | 63.1 | N 3557 (4) | 73.0 | 88.9 | I 4296 (5) | 86.3 | 115.3 | N 5128 (9) | |
| 3 | –27.7 | –17.0 | 83.0 | 9.6 | 3.5 | – | 16.7 | 9.3 | – | 39.2 | 46.3 | – | 87.1 | 46.2 | – | 90.7 | 69.2 | N 1316 (5) | 97.4 | 81.7 | – | |
| 4 | –34.4 | 13.0 | 63.0 | 8.2 | 3.0 | – | 9.9 | 11.4 | – | 65.0 | 44.9 | N 3557 (8) | 62.9 | 37.5 | N 3557 (4) | 60.2 | 69.4 | N 4760 (11) | 102.2 | 104.8 | N 5128 (7) | |
| 5 | –75.6 | –78.6 | 84.0 | 3.1 | 5.0 | – | 4.1 | 8.8 | – | 28.6 | 36.6 | – | 34.9 | 41.9 | N 1316 (6) | 49.5 | 54.4 | – | 61.0 | 66.0 | N 1316 (6) | |
| 6 | 58.8 | –42.4 | 71.0 | 3.9 | 2.9 | – | 6.3 | 6.2 | – | 36.1 | 46.2 | – | 58.5 | 52.4 | – | 93.7 | 84.5 | – | 101.8 | 89.9 | – | |
| 7 | –52.8 | 14.1 | 58.0 | 1.1 | 2.0 | N 5128 (12) | 2.0 | 4.1 | N 5128 (17) | 17.7 | 13.4 | I 4296 (7) | 32.4 | 41.9 | N 4760 (4) | 54.3 | 93.2 | N 5128 (6) | 82.7 | 107.6 | W 4452 (7) | |
| 8 | 4.2 | –54.9 | 57.0 | 41.0 | 34.6 | – | 40.5 | 28.0 | – | 71.6 | 44.4 | – | 89.7 | 60.2 | – | 96.9 | 68.3 | – | 103.8 | 91.1 | N 1316 (4) | |
| 9 | 48.8 | –28.7 | 59.0 | 6.3 | 5.0 | – | 12.6 | 8.3 | – | 69.9 | 44.5 | – | 113.4 | 70.8 | – | 122.4 | 76.0 | – | 144.1 | 94.8 | – | |
| 10 | –103.7 | –10.3 | 84.0 | 4.4 | 2.3 | – | 8.7 | 5.7 | – | 43.1 | 25.2 | – | 35.1 | 48.7 | – | 76.2 | 130.3 | – | 86.3 | 125.6 | – | |
| 11 | –165.9 | –46.9 | 85.0 | 4.7 | 2.0 | – | 10.1 | 3.8 | – | 38.2 | 28.1 | N 1316 (4) | 52.5 | 42.0 | – | 37.3 | 74.8 | – | 46.6 | 91.4 | – | |
| 12 | –27.6 | –16.5 | 59.0 | 11.2 | 4.8 | – | 24.2 | 29.5 | – | 75.0 | 49.6 | – | 86.2 | 55.0 | – | 91.1 | 82.7 | N 5128 (4) | 104.7 | 102.6 | – | |
| 13 | –52.3 | 7.3 | 79.0 | 3.3 | 2.0 | – | 5.3 | 4.4 | N 5128 (14) | 13.4 | 18.9 | N 5128 (14) | 49.8 | 59.6 | I 4296 (9) | 28.8 | 59.5 | I 4296 (6) | 38.4 | 80.6 | I 4296 (9) | |
| 14 | 88.8 | –47.1 | 83.0 | 4.5 | 2.8 | N 7626 (11) | 8.4 | 7.2 | – | 16.7 | 42.5 | – | 65.3 | 74.8 | N 7626 (5) | 84.6 | 71.3 | – | 95.6 | 67.9 | – | |
| 15 | –170.6 | –45.7 | 69.0 | 6.0 | 2.0 | – | 12.5 | 5.4 | – | 48.8 | 33.7 | – | 65.4 | 46.0 | – | 37.6 | 86.0 | – | 34.8 | 86.8 | – | |
| 16 | –51.2 | 17.2 | 69.0 | 0.6 | 1.9 | N 5128 (35) | 2.3 | 3.5 | N 5128 (24) | 15.8 | 12.6 | N 5128 (8) | 38.0 | 37.3 | I 4296 (6) | 67.1 | 86.4 | N 4760 (4) | 47.6 | 77.9 | N 5090 (8) | |
| 17 | –57.2 | 41.8 | 148.0 | 1.7 | 0.6 | – | 3.5 | 1.3 | – | 10.6 | 4.4 | – | 15.0 | 6.9 | N 3557 (6) | 14.9 | 11.2 | N 3557 (16) | 16.7 | 15.0 | N 3557 (22) | |
| 18 | 63.5 | –40.2 | 58.0 | 4.2 | 3.4 | – | 9.5 | 7.8 | – | 70.8 | 54.6 | – | 93.1 | 61.2 | – | 107.5 | 80.3 | N 1316 (4) | 109.4 | 78.3 | – | |
| 19 | –51.4 | 19.2 | 70.0 | 1.2 | 1.9 | N 5090 (35) | 2.2 | 3.4 | N 5090 (22) | 11.8 | 14.0 | N 5128 (7) | 30.8 | 40.5 | N 5128 (5) | 50.5 | 70.3 | N 4760 (9) | 62.0 | 88.7 | I 4296 (7) | |
| 20 | –109.4 | 23.8 | 64.0 | 6.1 | 2.2 | – | 12.6 | 4.9 | – | 53.5 | 12.3 | I 4296 (8) | 23.5 | 67.7 | I 4296 (4) | 51.3 | 123.7 | N 5090 (4) | 83.4 | 124.1 | N 5128 (6) | |
| 21 | –163.8 | –54.4 | 78.0 | 5.3 | 2.2 | – | 11.1 | 4.5 | – | 41.2 | 29.3 | – | 57.9 | 42.7 | – | 42.9 | 68.7 | – | 36.5 | 98.4 | – | |
| 22 | –41.7 | 5.9 | 64.0 | 5.7 | 2.8 | W 4452 (8) | 8.0 | 6.9 | W 4452 (4) | 34.9 | 32.4 | N 3557 (11) | 56.1 | 57.9 | – | 46.5 | 68.8 | N 5128 (9) | 118.2 | 118.8 | N 5128 (7) | |
| 23 | 12.1 | –49.0 | 90.0 | 4.9 | 5.3 | – | 60.8 | 57.3 | – | 69.7 | 37.6 | – | 81.0 | 51.6 | – | 88.2 | 59.3 | – | 102.6 | 63.3 | N 1316 (5) | |
| 24 | –21.8 | 54.1 | 71.0 | 2.7 | 1.4 | – | 6.4 | 3.3 | – | 47.3 | 11.3 | – | 50.0 | 16.9 | – | 42.7 | 20.6 | N 4261 (12) | 35.3 | 26.9 | N 4760 (13) | |
| 25 | –65.1 | 34.5 | 80.0 | 1.3 | 1.3 | – | 2.7 | 2.0 | – | 5.1 | 8.4 | – | 5.2 | 16.2 | N 3557 (8) | 7.4 | 35.8 | I 4296 (11) | 18.6 | 53.3 | N 5128 (16) | |
| 26 | –125.2 | –7.7 | 69.0 | 5.7 | 3.0 | – | 11.6 | 5.1 | – | 58.1 | 25.5 | – | 38.4 | 66.4 | – | 60.9 | 116.3 | – | 48.3 | 108.1 | – | |
Notes. This table summarizes the results of our Monte Carlo simulations for each PAO-detected UHECR within the BS-A model of the Galactic Magnetic Field. The first four columns specify a UHECR index number, the arrival direction at the observatory in Galactic coordinates, and the energy in EeV used for the UHECR. The remaining columns summarize the results for the six compositions for UHECRs simulated. For each composition, we list the average (first column for each composition) and rms (second column for each composition) of the 50 deflection angles, corresponding to the fifty Monte Carlo simulations. The deflection angle is the angular distance between the earth-arrival direction and the outside-the-Galaxy arrival direction. In the third column for each composition, we list the nearby extended radiogalaxy that most closely matches the 50 outside-the-Galaxy arrival directions of the UHECR and, in parenthesis, the number of outside-the-Galaxy arrival directions matched to this nearby extended radiogalaxy (maximum 50).
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