Table A.1
Diagnostics for all single age simulations with input observed MDF compared to observations.
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) |
| simulation | age | χ 2 | χ 2 | χ 2 |
|
|
simulation | age | χ 2 | χ 2 | χ 2 |
|
|
| ID | (Gyr) | CMD | LFI | LFV | RC | AGBb | ID | (Gyr) | CMD | LFI | LFV | RC | AGBb |
|
|
|||||||||||||
| aen015 | 13.0 | 108.7 | 73.7 | 52.2 | 29.0 | 8.9 | sol015 | 13.0 | 151.0 | 58.5 | 57.5 | 22.5 | 8.7 |
| aen020 | 13.0 | 104.4 | 65.5 | 42.8 | 28.6 | 6.1 | sol020 | 13.0 | 150.9 | 72.4 | 69.2 | 28.3 | 9.6 |
| aen021 | 12.5 | 94.7 | 58.3 | 44.2 | 21.5 | 8.2 | sol021 | 12.5 | 142.3 | 52.6 | 51.0 | 17.5 | 9.3 |
| aen022 | 12.0 | 76.4 | 36.2 | 25.8 | 8.4 | 5.3 | sol022 | 12.0 | 128.0 | 53.7 | 51.4 | 15.2 | 9.8 |
| aen023 | 11.5 | 75.3 | 42.7 | 34.4 | 5.1 | 7.5 | sol023 | 11.5 | 115.6 | 53.9 | 47.6 | 6.2 | 11.0 |
| aen018 | 11.0 | 65.6 | 53.6 | 40.5 | –0.9 | 8.8 | sol018 | 11.0 | 107.2 | 48.4 | 36.7 | –3.7 | 9.1 |
| aen024 | 11.0 | 66.2 | 55.3 | 39.1 | 1.1 | 7.4 | sol024 | 11.0 | 110.4 | 49.8 | 41.7 | –1.4 | 10.5 |
| aen025 | 10.5 | 65.2 | 55.7 | 34.5 | –10.6 | 7.0 | sol025 | 10.5 | 108.0 | 52.4 | 32.9 | –10.9 | 8.0 |
| aen016 | 10.0 | 67.1 | 72.4 | 41.0 | –10.1 | 7.4 | sol016 | 10.0 | 105.0 | 60.3 | 32.7 | –13.4 | 11.0 |
| aen017 | 10.0 | 67.7 | 74.1 | 39.3 | –9.4 | 8.6 | sol017 | 10.0 | 107.7 | 56.2 | 32.0 | –15.0 | 9.2 |
| aen026 | 10.0 | 68.9 | 69.9 | 38.4 | –11.5 | 8.4 | sol026 | 10.0 | 108.7 | 62.4 | 37.1 | –7.7 | 8.4 |
| aen027 | 9.5 | 76.0 | 82.7 | 39.0 | –15.0 | 9.1 | sol027 | 9.5 | 109.8 | 65.2 | 30.4 | –17.2 | 8.2 |
| aen028 | 9.0 | 81.4 | 114.4 | 50.9 | –7.9 | 7.5 | sol028 | 9.0 | 111.7 | 73.5 | 29.4 | –16.9 | 8.9 |
| aen029 | 8.5 | 90.3 | 131.3 | 54.9 | –6.8 | 8.1 | sol029 | 8.5 | 115.9 | 85.4 | 29.0 | –16.2 | 8.0 |
| aen030 | 8.0 | 95.7 | 140.4 | 56.5 | –0.5 | 6.9 | sol030 | 8.0 | 115.1 | 78.9 | 22.9 | –15.8 | 7.4 |
| aen031 | 7.5 | 107.1 | 158.6 | 68.0 | 6.5 | 8.4 | sol031 | 7.5 | 115.4 | 96.7 | 26.6 | –10.9 | 8.9 |
| aen019 | 7.0 | 130.7 | 199.3 | 83.8 | 13.2 | 7.6 | sol019 | 7.0 | 116.6 | 113.3 | 34.3 | –3.3 | 8.7 |
| aen032 | 7.0 | 128.6 | 210.7 | 94.6 | 17.0 | 10.0 | sol032 | 7.0 | 116.1 | 110.9 | 32.4 | –6.2 | 8.8 |
| aen033 | 6.5 | 149.6 | 225.3 | 94.9 | 19.1 | 8.2 | sol033 | 6.5 | 122.0 | 131.9 | 36.8 | –0.1 | 7.8 |
| aen034 | 6.0 | 173.0 | 241.4 | 103.5 | 24.2 | 6.8 | sol034 | 6.0 | 133.1 | 146.5 | 41.3 | 3.2 | 8.7 |
| aen035 | 5.5 | 210.8 | 292.7 | 125.1 | 29.4 | 7.3 | sol035 | 5.5 | 140.5 | 166.8 | 47.7 | 9.6 | 7.3 |
| aen036 | 5.0 | 237.3 | 331.6 | 157.7 | 39.1 | 8.0 | sol036 | 5.0 | 153.4 | 207.5 | 68.6 | 19.0 | 6.6 |
| aen037 | 4.5 | 285.6 | 370.8 | 180.1 | 45.2 | 7.7 | sol037 | 4.5 | 177.6 | 254.1 | 90.7 | 26.3 | 9.7 |
| aen038 | 4.0 | 320.0 | 419.4 | 226.8 | 51.9 | 7.1 | sol038 | 4.0 | 199.7 | 282.2 | 105.4 | 30.6 | 7.1 |
| aen039 | 3.5 | 375.1 | 513.2 | 282.4 | 58.7 | 7.3 | sol039 | 3.5 | 231.7 | 349.8 | 147.8 | 38.6 | 6.7 |
| aen040 | 3.0 | 423.9 | 608.7 | 364.8 | 66.8 | 8.1 | sol040 | 3.0 | 274.4 | 426.2 | 210.5 | 48.1 | 6.1 |
| aen041 | 2.5 | 511.2 | 684.6 | 428.0 | 73.6 | 7.5 | sol041 | 2.5 | 347.8 | 526.8 | 275.0 | 59.7 | 7.5 |
| aen042 | 2.0 | 643.7 | 801.0 | 568.3 | 80.9 | 10.2 | sol042 | 2.0 | 427.7 | 640.7 | 379.7 | 68.7 | 6.7 |
Notes. 
in Cols. 6, 7, 13, and 14 is the number difference between the observed and simulated stars in the parts of the CMD that are dominated by the RC (Cols. 6, 13) or AGBb stars (Cols. 7, 14), weighted by the Poissonian fluctuation in the number of stars expected from the observations. The first set (left) is for the models that included alpha enhancement (aen*), the second (right) for solar scaled models (sol*). The preferred models, those having smallest χ2 (or ΔN close to 0), for each diagnostic are indicated with bold-faced fonts.
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