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Table 8.
Derived binary-fractions, fder(q > 0.5), fder(tot)mf and fder(tot)mc (see Eq. (8); Cols. 2–7, 8–13, and 14–19), and the corresponding FF indicator 
for the final binary fraction profile (see the text below Eq. (7)).
| No: Name (i) | fder(q > 0.5),  |
fder(tot)mf,  |
fder(tot)mc,  |
|---|---|---|---|
| P02 U17 S05-1 S05-2 S05-3 | P02 U17 S05-1 S05-2 S05-3 | P02 U17 S05-1 S05-2 S05-3 | |
| (1) | (2) (3) (4) (5) (6) (7) | (8) (9) (10) (11) (12) (13) | (14) (15) (16) (17) (18) (19) |
| 3: NGC 104* | ........... 0.0425 0.0412 ........... ........... 1 | ........... 0.0989 0.0973 ........... ........... 3 | ........... 0.0267 0.0374 ........... ........... 1 |
| 5: NGC 362 | ........... 0.0507 ........... ........... ........... 3 | ........... 0.0597 ........... ........... ........... 1 | ........... 0.0478 ........... ........... ........... 1 |
| 6: NGC 1261 | ........... 0.0247 ........... ........... ........... 1 | ........... 0.0496 ........... ........... ........... 1 | ........... 0.0496 ........... ........... ........... 1 |
| 7: NGC 1851* | ........... 0.0354 0.0358 ........... ........... 1 | ........... 0.0282 0.0227 ........... ........... 1 | ........... -.0029 -.0164 ........... ........... 1 |
| 8: NGC 2298* | ........... ........... 0.0810 0.0818 ........... 1 | ........... ........... 0.1619 0.1635 ........... 1 | ........... ........... 0.1619 0.1635 ........... 1 |
| 9: NGC 3201* | ........... 0.0663 0.0618 0.0618 ........... 0 | ........... 0.1336 0.1245 0.1245 ........... 0 | ........... 0.1336 0.1245 0.1245 ........... 0 |
| 10: NGC 4147 | ........... 0.0422 ........... ........... ........... 1 | ........... 0.0843 ........... ........... ........... 1 | ........... 0.0843 ........... ........... ........... 1 |
| 11: NGC 4590 | ........... 0.0726 ........... ........... ........... 1 | ........... 0.1023 ........... ........... ........... 1 | ........... 0.0763 ........... ........... ........... 1 |
| 12: NGC 4833 | ........... 0.0365 ........... ........... ........... 0 | ........... 0.0731 ........... ........... ........... 0 | ........... 0.0731 ........... ........... ........... 0 |
| 13: NGC 5024 | ........... 0.0269 ........... ........... ........... 1 | ........... 0.0528 ........... ........... ........... 2 | ........... 0.0528 ........... ........... ........... 2 |
| 15: NGC 5272 | ........... 0.0602 ........... ........... ........... 1 | ........... 0.0628 ........... ........... ........... 1 | ........... 0.0915 ........... ........... ........... 1 |
| 16: NGC 5286 | x x x x x x | x x x x x x | x x x x x x |
| 19: NGC 5904* | ........... 0.0564 0.0515 0.0522 ........... 1 | ........... 0.0312 0.0327 0.0325 ........... 1 | ........... 0.0329 0.0340 0.0339 ........... 1 |
| 20: NGC 5927* | 0.0577 0.0516 0.0461 0.0461 0.0476 0 | 0.0260 0.0375 0.0479 0.0479 0.0451 1 | -.0168 0.0063 0.0278 0.0278 0.0220 1 |
| 21: NGC 5986* | ........... 0.0041 0.0042 ........... ........... 2 | ........... 0.0092 0.0095 ........... ........... 2 | ........... 0.0092 0.0095 ........... ........... 2 |
| 22: NGC 6093 | ........... 0.0626 ........... ........... ........... 0 | ........... 0.0261 ........... ........... ........... 1 | ........... 0.0358 ........... ........... ........... 1 |
| 24: NGC 6121* | ........... 0.0725 0.0554 ........... ........... 1 | ........... 0.1707 0.1445 ........... ........... 1 | ........... 0.0010 0.0013 ........... ........... 3 |
| 26: NGC 6171* | ........... 0.0990 0.0852 0.0849 ........... 1 | ........... 0.1981 0.1706 0.1699 ........... 1 | ........... 0.1981 0.1706 0.1699 ........... 1 |
| 28: NGC 6218* | 0.0478 0.0454 0.0398 ........... ........... 1 | 0.1073 0.1005 0.0891 ........... ........... 0 | 0.0419 0.0456 0.0542 ........... ........... 1 |
| 29: NGC 6254* | ........... 0.0405 0.0337 ........... ........... 1 | ........... 0.0819 0.0680 ........... ........... 1 | ........... 0.0819 0.0680 ........... ........... 1 |
| 31: NGC 6352* | ........... 0.0776 0.0702 ........... ........... 1 | ........... 0.1502 0.1356 ........... ........... 1 | ........... 0.0222 -.0024 ........... ........... 1 |
| 32: NGC 6362* | ........... 0.0634 0.0471 ........... ........... 1 | ........... 0.1408 0.1024 ........... ........... 1 | ........... 0.1118 0.1007 ........... ........... 3 |
| 34: NGC 6388 | x x x x x x | x x x x x x | x x x x x x |
| 35: NGC 6397 | ........... 0.0378 ........... ........... ........... 0 | ........... 0.0690 ........... ........... ........... 0 | ........... -.0117 ........... ........... ........... 1 |
| 36: NGC 6441 | x x x x x x | x x x x x x | x x x x x x |
| 39: NGC 6541 | ........... 0.0485 ........... ........... ........... 0 | ........... 0.0228 ........... ........... ........... 1 | ........... -.0089 ........... ........... ........... 1 |
| 40: NGC 6584 | ........... 0.0441 ........... ........... ........... 1 | ........... 0.0891 ........... ........... ........... 1 | ........... 0.0891 ........... ........... ........... 1 |
| 41: NGC 6624* | 0.0113 0.0114 0.0113 0.0114 ........... 1 | 0.0084 0.0251 0.0093 0.0134 ........... 1 | 0.0452 0.0485 0.0456 0.0468 ........... 1 |
| 42: NGC 6637* | 0.0428 0.0382 0.0374 ........... ........... 1 | 0.0707 0.0673 0.0667 ........... ........... 1 | 0.0101 0.0198 0.0223 ........... ........... 1 |
| 43: NGC 6652* | ........... 0.0468 0.0519 0.0519 ........... 1 | ........... 0.1089 0.1122 0.1122 ........... 1 | ........... 0.0440 0.0456 0.0456 ........... 1 |
| 44: NGC 6656 | ........... 0.0236 ........... ........... ........... 0 | ........... 0.1051 ........... ........... ........... 1 | ........... -.0279 ........... ........... ........... 1 |
| 45: NGC 6681 | ........... 0.0264 ........... ........... ........... 0 | ........... 0.0538 ........... ........... ........... 0 | ........... 0.0538 ........... ........... ........... 0 |
| 46: NGC 6723* | ........... 0.0537 0.0443 ........... ........... 1 | ........... 0.0746 0.0627 ........... ........... 1 | ........... 0.0530 0.0638 ........... ........... 1 |
| 47: NGC 6752* | ........... 0.0087 0.0093 ........... ........... 1 | ........... 0.0236 0.0256 ........... ........... 1 | ........... 0.0083 0.0105 ........... ........... 1 |
| 49: NGC 6809 | ........... 0.0311 ........... ........... ........... 1 | ........... 0.0002 ........... ........... ........... 1 | ........... 0.2622 ........... ........... ........... 1 |
| 50: NGC 6838 | ........... 0.1583 ........... ........... ........... 1 | ........... 0.3176 ........... ........... ........... 1 | ........... 0.3176 ........... ........... ........... 1 |
| 51: NGC 6934 | ........... 0.0319 ........... ........... ........... 3 | ........... 0.0638 ........... ........... ........... 3 | ........... 0.0638 ........... ........... ........... 3 |
| 52: NGC 6981 | 0.0749 ........... ........... ........... ........... 1 | 0.0875 ........... ........... ........... ........... 1 | 0.0716 ........... ........... ........... ........... 1 |
| 53: NGC 7078* | ........... 0.0438 0.0455 0.0440 ........... 1 | ........... 0.0168 0.0183 0.0170 ........... 1 | ........... 0.0161 0.0171 0.0162 ........... 1 |
| 54: NGC 7089* | ........... 0.0390 0.0381 ........... ........... 0 | ........... 0.0790 0.0771 ........... ........... 0 | ........... 0.0790 0.0771 ........... ........... 0 |
| 55: NGC 7099 | ........... 0.0274 ........... ........... ........... 1 | ........... 0.0272 ........... ........... ........... 1 | ........... 0.0036 ........... ........... ........... 1 |
| 63: NGC 7006 | x x x x x x | x x x x x x | x x x x x x |
| 68: NGC 2808* | ........... 0.0091 0.0091 0.0091 ........... 3 | x x x x x x | x x x x x x |
| 69: NGC 5139 | x x x x x x | x x x x x x | x x x x x x |
Notes. For each type, there are six columns, with the first five columns are the binary fraction within the equivalent region of the P02, U17, S05-1, -2, and -3 observations, and the last column is 
. In this table, ‘..’ indicates that GC has no spectroscopic observations (see Col. 3 of Tables 5 and 6); ‘x’ indicates that GC has nbin ≤ 2 (see the text below Eq. (4)). The GC name ending with a star refers to the new GC sample.
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