Results of our simulations for the system Kepler-1625 considering the star. For each column, we have the systems separated by the mass of the co-orbital companion (M2), and the number and percentage of systems with collisions between the planet and the co-orbital companion (Coll. Mp − M2), collisions between the satellites (Coll. M1 − M2), collisions between the planet and Kepler-1625 b-I (Coll. Mp − M2), ejections of the co-orbital companion (M2 Ejected), ejections of Kepler-1625 b-I (M1 Ejected), and ploonets. In the last row, we have the summation of all simulated cases and their respective percentages.
| M2 . | Coll. Mp − M2 . | Coll. M1 − M2 . | Coll. Mp − M1 . | M2 Ejected . | M1 Ejected . | Ploonet . |
|---|---|---|---|---|---|---|
| M⊕ . | . | . | . | . | . | . |
| 0.107 | |$26\,\,(\sim 42.6\,{\rm per\,cent})$| | |$28\,\,(\sim 45.9\,\rm per\,cent)$| | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | − | − | − |
| 1.0 | |$24\,\,(\sim 39.3\,{\rm per\,cent})$| | |$31\,\,(\sim 50.8\,{\rm per\,cent})$| | |$6\,\,(\sim 9.8\,{\rm per\,cent})$| | − | − | − |
| 2.0 | |$24\,\,(\sim 39.3\,{\rm per\,cent})$| | |$33\,\,(\sim 54.1\,{\rm per\,cent})$| | |$4\,\,(\sim 6.6\,{\rm per\,cent})$| | − | − | − |
| 3.0 | |$22\,\,(\sim 36.1\,{\rm per\,cent})$| | |$33\,\,(\sim 54.1\,\rm per\,cent)$| | |$5\,\,(\sim 8.2\,\rm per\,cent)$| | − | − | |$1\,\,(\sim 1.6\,\rm per\,cent)$| |
| 4.0 | |$20\,\,(\sim 32.8\,\rm per\,cent)$| | |$32\,\,(\sim 52.5\,\rm per\,cent)$| | |$9\,\,(\sim 14.8\,\rm per\,cent)$| | − | − | − |
| 5.0 | |$24\,\,(\sim 39.3\,\rm per\,cent)$| | |$29\,\,(\sim 47.5\,\rm per\,cent)$| | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − | − |
| 6.0 | |$23\,\,(\sim 37.7\,\rm per\,cent)$| | |$28\,\,(\sim 45.9\,\rm per\,cent)$| | |$8\,\,(\sim 13.1\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | − | − |
| 7.0 | |$16\,\,(\sim 26.2\,\rm per\,cent)$| | |$35\,\,(\sim 57.4\,\rm per\,cent)$| | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | − | − |
| 8.0 | |$16\,\,(\sim 26.2\,\rm per\,cent)$| | |$32\,\,(\sim 52.4\,\rm per\,cent)$| | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | |$9\,\,(\sim 14.8\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − |
| 9.0 | |$16\,\,(\sim 26.2\,\rm per\,cent)$| | |$36\,\,(\sim 59.0\,\rm per\,cent)$| | |$4\,\,(\sim 6.6\,\rm per\,cent)$| | |$4\,\,(\sim 6.6\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − |
| 10.0 | |$10\,\,(\sim 16.4\,\rm per\,cent)$| | |$42\,\,(\sim 68.9\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | |$6\,\,(\sim 9.8\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − |
| 11.0 | |$14\,\,(\sim 22.9\,\rm per\,cent)$| | |$36\,\,(\sim 59.0\,\rm per\,cent)$| | |$5\,\,(\sim 8.2\,\rm per\,cent)$| | |$5\,\,(\sim 8.2\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − |
| 12.0 | |$12\,\,(\sim 19.7\,\rm per\,cent)$| | |$43\,\,(\sim 70.5\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | |$1\,\,(\sim 4.9\,\rm per\,cent)$| | − |
| 13.0 | |$10\,\,(\sim 16.4\,\rm per\,cent)$| | |$39\,\,(\sim 63.9\,\rm per\,cent)$| | − | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | |$5\,\,(\sim 8.2\,\rm per\,cent)$| | − |
| 14.0 | |$13\,\,(\sim 21.3\,\rm per\,cent)$| | |$36\,\,(\sim 59.0\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | − |
| 15.0 | |$17\,\,(\sim 27.9\,\rm per\,cent)$| | |$29\,\,(\sim 47.5\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | |$8\,\,(\sim 13.1\,\rm per\,cent)$| | |$6\,\,(\sim 9.8\,\rm per\,cent)$| | − |
| 16.0 | |$10\,\,(\sim 16.4\,\rm per\,cent)$| | |$37\,\,(\sim 60.7\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | |$9\,\,(\sim 14.8\,\rm per\,cent)$| | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | − |
| 17.15 | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | |$45\,\,(\sim 73.8\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | |$10\,\,(\sim 16.4\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | − |
| Total | |$\mathbf {300\,\,(\sim 27.3 \,\rm per\,cent)}$| | |$\mathbf {624\,\,(\sim 56.8\,\rm per\,cent)}$| | |$\mathbf {75\,\,(\sim 6.8\,\rm per\,cent)}$| | |$\mathbf {72\,\,(\sim 6.6\,\rm per\,cent)}$| | |$\mathbf {26\,\,(\sim 2.4\,\rm per\,cent)}$| | |$\mathbf {1\,\,(\sim 0.09\,\rm per\,cent)}$| |
| M2 . | Coll. Mp − M2 . | Coll. M1 − M2 . | Coll. Mp − M1 . | M2 Ejected . | M1 Ejected . | Ploonet . |
|---|---|---|---|---|---|---|
| M⊕ . | . | . | . | . | . | . |
| 0.107 | |$26\,\,(\sim 42.6\,{\rm per\,cent})$| | |$28\,\,(\sim 45.9\,\rm per\,cent)$| | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | − | − | − |
| 1.0 | |$24\,\,(\sim 39.3\,{\rm per\,cent})$| | |$31\,\,(\sim 50.8\,{\rm per\,cent})$| | |$6\,\,(\sim 9.8\,{\rm per\,cent})$| | − | − | − |
| 2.0 | |$24\,\,(\sim 39.3\,{\rm per\,cent})$| | |$33\,\,(\sim 54.1\,{\rm per\,cent})$| | |$4\,\,(\sim 6.6\,{\rm per\,cent})$| | − | − | − |
| 3.0 | |$22\,\,(\sim 36.1\,{\rm per\,cent})$| | |$33\,\,(\sim 54.1\,\rm per\,cent)$| | |$5\,\,(\sim 8.2\,\rm per\,cent)$| | − | − | |$1\,\,(\sim 1.6\,\rm per\,cent)$| |
| 4.0 | |$20\,\,(\sim 32.8\,\rm per\,cent)$| | |$32\,\,(\sim 52.5\,\rm per\,cent)$| | |$9\,\,(\sim 14.8\,\rm per\,cent)$| | − | − | − |
| 5.0 | |$24\,\,(\sim 39.3\,\rm per\,cent)$| | |$29\,\,(\sim 47.5\,\rm per\,cent)$| | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − | − |
| 6.0 | |$23\,\,(\sim 37.7\,\rm per\,cent)$| | |$28\,\,(\sim 45.9\,\rm per\,cent)$| | |$8\,\,(\sim 13.1\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | − | − |
| 7.0 | |$16\,\,(\sim 26.2\,\rm per\,cent)$| | |$35\,\,(\sim 57.4\,\rm per\,cent)$| | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | − | − |
| 8.0 | |$16\,\,(\sim 26.2\,\rm per\,cent)$| | |$32\,\,(\sim 52.4\,\rm per\,cent)$| | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | |$9\,\,(\sim 14.8\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − |
| 9.0 | |$16\,\,(\sim 26.2\,\rm per\,cent)$| | |$36\,\,(\sim 59.0\,\rm per\,cent)$| | |$4\,\,(\sim 6.6\,\rm per\,cent)$| | |$4\,\,(\sim 6.6\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − |
| 10.0 | |$10\,\,(\sim 16.4\,\rm per\,cent)$| | |$42\,\,(\sim 68.9\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | |$6\,\,(\sim 9.8\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − |
| 11.0 | |$14\,\,(\sim 22.9\,\rm per\,cent)$| | |$36\,\,(\sim 59.0\,\rm per\,cent)$| | |$5\,\,(\sim 8.2\,\rm per\,cent)$| | |$5\,\,(\sim 8.2\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − |
| 12.0 | |$12\,\,(\sim 19.7\,\rm per\,cent)$| | |$43\,\,(\sim 70.5\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | |$1\,\,(\sim 4.9\,\rm per\,cent)$| | − |
| 13.0 | |$10\,\,(\sim 16.4\,\rm per\,cent)$| | |$39\,\,(\sim 63.9\,\rm per\,cent)$| | − | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | |$5\,\,(\sim 8.2\,\rm per\,cent)$| | − |
| 14.0 | |$13\,\,(\sim 21.3\,\rm per\,cent)$| | |$36\,\,(\sim 59.0\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | − |
| 15.0 | |$17\,\,(\sim 27.9\,\rm per\,cent)$| | |$29\,\,(\sim 47.5\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | |$8\,\,(\sim 13.1\,\rm per\,cent)$| | |$6\,\,(\sim 9.8\,\rm per\,cent)$| | − |
| 16.0 | |$10\,\,(\sim 16.4\,\rm per\,cent)$| | |$37\,\,(\sim 60.7\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | |$9\,\,(\sim 14.8\,\rm per\,cent)$| | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | − |
| 17.15 | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | |$45\,\,(\sim 73.8\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | |$10\,\,(\sim 16.4\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | − |
| Total | |$\mathbf {300\,\,(\sim 27.3 \,\rm per\,cent)}$| | |$\mathbf {624\,\,(\sim 56.8\,\rm per\,cent)}$| | |$\mathbf {75\,\,(\sim 6.8\,\rm per\,cent)}$| | |$\mathbf {72\,\,(\sim 6.6\,\rm per\,cent)}$| | |$\mathbf {26\,\,(\sim 2.4\,\rm per\,cent)}$| | |$\mathbf {1\,\,(\sim 0.09\,\rm per\,cent)}$| |
Results of our simulations for the system Kepler-1625 considering the star. For each column, we have the systems separated by the mass of the co-orbital companion (M2), and the number and percentage of systems with collisions between the planet and the co-orbital companion (Coll. Mp − M2), collisions between the satellites (Coll. M1 − M2), collisions between the planet and Kepler-1625 b-I (Coll. Mp − M2), ejections of the co-orbital companion (M2 Ejected), ejections of Kepler-1625 b-I (M1 Ejected), and ploonets. In the last row, we have the summation of all simulated cases and their respective percentages.
| M2 . | Coll. Mp − M2 . | Coll. M1 − M2 . | Coll. Mp − M1 . | M2 Ejected . | M1 Ejected . | Ploonet . |
|---|---|---|---|---|---|---|
| M⊕ . | . | . | . | . | . | . |
| 0.107 | |$26\,\,(\sim 42.6\,{\rm per\,cent})$| | |$28\,\,(\sim 45.9\,\rm per\,cent)$| | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | − | − | − |
| 1.0 | |$24\,\,(\sim 39.3\,{\rm per\,cent})$| | |$31\,\,(\sim 50.8\,{\rm per\,cent})$| | |$6\,\,(\sim 9.8\,{\rm per\,cent})$| | − | − | − |
| 2.0 | |$24\,\,(\sim 39.3\,{\rm per\,cent})$| | |$33\,\,(\sim 54.1\,{\rm per\,cent})$| | |$4\,\,(\sim 6.6\,{\rm per\,cent})$| | − | − | − |
| 3.0 | |$22\,\,(\sim 36.1\,{\rm per\,cent})$| | |$33\,\,(\sim 54.1\,\rm per\,cent)$| | |$5\,\,(\sim 8.2\,\rm per\,cent)$| | − | − | |$1\,\,(\sim 1.6\,\rm per\,cent)$| |
| 4.0 | |$20\,\,(\sim 32.8\,\rm per\,cent)$| | |$32\,\,(\sim 52.5\,\rm per\,cent)$| | |$9\,\,(\sim 14.8\,\rm per\,cent)$| | − | − | − |
| 5.0 | |$24\,\,(\sim 39.3\,\rm per\,cent)$| | |$29\,\,(\sim 47.5\,\rm per\,cent)$| | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − | − |
| 6.0 | |$23\,\,(\sim 37.7\,\rm per\,cent)$| | |$28\,\,(\sim 45.9\,\rm per\,cent)$| | |$8\,\,(\sim 13.1\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | − | − |
| 7.0 | |$16\,\,(\sim 26.2\,\rm per\,cent)$| | |$35\,\,(\sim 57.4\,\rm per\,cent)$| | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | − | − |
| 8.0 | |$16\,\,(\sim 26.2\,\rm per\,cent)$| | |$32\,\,(\sim 52.4\,\rm per\,cent)$| | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | |$9\,\,(\sim 14.8\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − |
| 9.0 | |$16\,\,(\sim 26.2\,\rm per\,cent)$| | |$36\,\,(\sim 59.0\,\rm per\,cent)$| | |$4\,\,(\sim 6.6\,\rm per\,cent)$| | |$4\,\,(\sim 6.6\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − |
| 10.0 | |$10\,\,(\sim 16.4\,\rm per\,cent)$| | |$42\,\,(\sim 68.9\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | |$6\,\,(\sim 9.8\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − |
| 11.0 | |$14\,\,(\sim 22.9\,\rm per\,cent)$| | |$36\,\,(\sim 59.0\,\rm per\,cent)$| | |$5\,\,(\sim 8.2\,\rm per\,cent)$| | |$5\,\,(\sim 8.2\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − |
| 12.0 | |$12\,\,(\sim 19.7\,\rm per\,cent)$| | |$43\,\,(\sim 70.5\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | |$1\,\,(\sim 4.9\,\rm per\,cent)$| | − |
| 13.0 | |$10\,\,(\sim 16.4\,\rm per\,cent)$| | |$39\,\,(\sim 63.9\,\rm per\,cent)$| | − | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | |$5\,\,(\sim 8.2\,\rm per\,cent)$| | − |
| 14.0 | |$13\,\,(\sim 21.3\,\rm per\,cent)$| | |$36\,\,(\sim 59.0\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | − |
| 15.0 | |$17\,\,(\sim 27.9\,\rm per\,cent)$| | |$29\,\,(\sim 47.5\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | |$8\,\,(\sim 13.1\,\rm per\,cent)$| | |$6\,\,(\sim 9.8\,\rm per\,cent)$| | − |
| 16.0 | |$10\,\,(\sim 16.4\,\rm per\,cent)$| | |$37\,\,(\sim 60.7\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | |$9\,\,(\sim 14.8\,\rm per\,cent)$| | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | − |
| 17.15 | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | |$45\,\,(\sim 73.8\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | |$10\,\,(\sim 16.4\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | − |
| Total | |$\mathbf {300\,\,(\sim 27.3 \,\rm per\,cent)}$| | |$\mathbf {624\,\,(\sim 56.8\,\rm per\,cent)}$| | |$\mathbf {75\,\,(\sim 6.8\,\rm per\,cent)}$| | |$\mathbf {72\,\,(\sim 6.6\,\rm per\,cent)}$| | |$\mathbf {26\,\,(\sim 2.4\,\rm per\,cent)}$| | |$\mathbf {1\,\,(\sim 0.09\,\rm per\,cent)}$| |
| M2 . | Coll. Mp − M2 . | Coll. M1 − M2 . | Coll. Mp − M1 . | M2 Ejected . | M1 Ejected . | Ploonet . |
|---|---|---|---|---|---|---|
| M⊕ . | . | . | . | . | . | . |
| 0.107 | |$26\,\,(\sim 42.6\,{\rm per\,cent})$| | |$28\,\,(\sim 45.9\,\rm per\,cent)$| | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | − | − | − |
| 1.0 | |$24\,\,(\sim 39.3\,{\rm per\,cent})$| | |$31\,\,(\sim 50.8\,{\rm per\,cent})$| | |$6\,\,(\sim 9.8\,{\rm per\,cent})$| | − | − | − |
| 2.0 | |$24\,\,(\sim 39.3\,{\rm per\,cent})$| | |$33\,\,(\sim 54.1\,{\rm per\,cent})$| | |$4\,\,(\sim 6.6\,{\rm per\,cent})$| | − | − | − |
| 3.0 | |$22\,\,(\sim 36.1\,{\rm per\,cent})$| | |$33\,\,(\sim 54.1\,\rm per\,cent)$| | |$5\,\,(\sim 8.2\,\rm per\,cent)$| | − | − | |$1\,\,(\sim 1.6\,\rm per\,cent)$| |
| 4.0 | |$20\,\,(\sim 32.8\,\rm per\,cent)$| | |$32\,\,(\sim 52.5\,\rm per\,cent)$| | |$9\,\,(\sim 14.8\,\rm per\,cent)$| | − | − | − |
| 5.0 | |$24\,\,(\sim 39.3\,\rm per\,cent)$| | |$29\,\,(\sim 47.5\,\rm per\,cent)$| | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − | − |
| 6.0 | |$23\,\,(\sim 37.7\,\rm per\,cent)$| | |$28\,\,(\sim 45.9\,\rm per\,cent)$| | |$8\,\,(\sim 13.1\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | − | − |
| 7.0 | |$16\,\,(\sim 26.2\,\rm per\,cent)$| | |$35\,\,(\sim 57.4\,\rm per\,cent)$| | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | − | − |
| 8.0 | |$16\,\,(\sim 26.2\,\rm per\,cent)$| | |$32\,\,(\sim 52.4\,\rm per\,cent)$| | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | |$9\,\,(\sim 14.8\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − |
| 9.0 | |$16\,\,(\sim 26.2\,\rm per\,cent)$| | |$36\,\,(\sim 59.0\,\rm per\,cent)$| | |$4\,\,(\sim 6.6\,\rm per\,cent)$| | |$4\,\,(\sim 6.6\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − |
| 10.0 | |$10\,\,(\sim 16.4\,\rm per\,cent)$| | |$42\,\,(\sim 68.9\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | |$6\,\,(\sim 9.8\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − |
| 11.0 | |$14\,\,(\sim 22.9\,\rm per\,cent)$| | |$36\,\,(\sim 59.0\,\rm per\,cent)$| | |$5\,\,(\sim 8.2\,\rm per\,cent)$| | |$5\,\,(\sim 8.2\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | − |
| 12.0 | |$12\,\,(\sim 19.7\,\rm per\,cent)$| | |$43\,\,(\sim 70.5\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | |$1\,\,(\sim 4.9\,\rm per\,cent)$| | − |
| 13.0 | |$10\,\,(\sim 16.4\,\rm per\,cent)$| | |$39\,\,(\sim 63.9\,\rm per\,cent)$| | − | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | |$5\,\,(\sim 8.2\,\rm per\,cent)$| | − |
| 14.0 | |$13\,\,(\sim 21.3\,\rm per\,cent)$| | |$36\,\,(\sim 59.0\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | |$7\,\,(\sim 11.5\,\rm per\,cent)$| | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | − |
| 15.0 | |$17\,\,(\sim 27.9\,\rm per\,cent)$| | |$29\,\,(\sim 47.5\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | |$8\,\,(\sim 13.1\,\rm per\,cent)$| | |$6\,\,(\sim 9.8\,\rm per\,cent)$| | − |
| 16.0 | |$10\,\,(\sim 16.4\,\rm per\,cent)$| | |$37\,\,(\sim 60.7\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | |$9\,\,(\sim 14.8\,\rm per\,cent)$| | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | − |
| 17.15 | |$3\,\,(\sim 4.9\,\rm per\,cent)$| | |$45\,\,(\sim 73.8\,\rm per\,cent)$| | |$1\,\,(\sim 1.6\,\rm per\,cent)$| | |$10\,\,(\sim 16.4\,\rm per\,cent)$| | |$2\,\,(\sim 3.3\,\rm per\,cent)$| | − |
| Total | |$\mathbf {300\,\,(\sim 27.3 \,\rm per\,cent)}$| | |$\mathbf {624\,\,(\sim 56.8\,\rm per\,cent)}$| | |$\mathbf {75\,\,(\sim 6.8\,\rm per\,cent)}$| | |$\mathbf {72\,\,(\sim 6.6\,\rm per\,cent)}$| | |$\mathbf {26\,\,(\sim 2.4\,\rm per\,cent)}$| | |$\mathbf {1\,\,(\sim 0.09\,\rm per\,cent)}$| |
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