Table 6.
Three observed regions for the 24 GCs (37 integrated spectral energy distributions) from the binary fraction sample matched with the S05 work.
| ID Name | ( , lH1,lH2) |
( , lH1,lH2) |
( , lH1,lH2) |
|---|---|---|---|
| (″, ″, ″) | (″, ″, ″) | (″, ″, ″) | |
| i | ( ) |
( ) |
( ) |
| (1) | (2) | (3) | (4) |
| 3 NGC 104 | 24.0 −25.0 25.0 | .. .. .. | .. .. .. |
| 7 NGC 1851 | 4.5 −9.0 9.0 | .. .. .. | .. .. ... |
| 8 NGC 2298 | 18.0 −24.0 20.0 | 18.0 −20.0 20.0 | .. .. .. |
| 9 NGC 3201 | 85.0 −85.0 85.0 | 85.0 −85.0 85.0 | .. .. .. |
| 16 NGC 5286 | 18.0 −20.0 20.0 | 18.0 −20.0 20.0 | 18.0 −20.0 23.0 |
| 19 NGC 5904 | 27.0 −27.0 30.0 | 22.5 −27.0 30.0 | .. .. .. |
| 20 NGC 5927 | 25.0 −29.0 29.0 | 25.0 −29.0 29.0 | 23.0 −25.0 25.0 |
| 21 NGC 5986 | 38.0 −32.0 42.0 | .. .. .. | .. .. .. |
| 24 NGC 6121 | 50.0 −50.0 50.0 | .. .. .. | .. .. .. |
| 26 NGC 6171 | 32.0 −32.0 36.0 | 32.0 −32.0 37.0 | .. .. .. |
| 28 NGC 6218 | 45.0 −45.0 45.0 | .. .. .. | .. .. .. |
| 29 NGC 6254 | 54.0 −54.0 54.0 | .. .. .. | .. .. .. |
| 31 NGC 6352 | 49.5 −50.0 50.0 | .. .. .. | .. .. .. |
| 32 NGC 6362 | 80.0 −80.0 80.0 | .. .. .. | .. .. .. |
| 34 NGC 6388 | 9.0 −10.0 10.0 | .. .. .. | .. .. .. |
| 36 NGC 6441 | 6.0 −10.0 10.0 | 6.0 −18.0 18.0 | .. .. .. |
| 41 NGC 6624 | 4.5 −7.0 5.0 | 4.5. −11.0 11.0 | .. .. .. |
| 42 NGC 6637 | 18.0 −20.0 20.0 | .. .. .. | .. .. .. |
| 43 NGC 6652 (a) | 4.5 −7.0 7.0 | 4.5 −7.0 7.0 | .. .. .. |
| 46 NGC 6723 | 54.0 −54.0 54.0 | .. .. .. | .. .. .. |
| 47 NGC 6752 | 9.0 −13.0 11.0 | .. .. .. | .. .. .. |
| 53 NGC 7078 | 4.5 −5.0 5.0 | 4.5 −20.0 20.0 | .. .. .. |
| 54 NGC 7089 | 18.0 −22.0 22.0 | .. .. .. | .. .. .. |
| 68 NGC 2808 | 15.0 −20.0 20.0 | 15.0 −17.0 15.0 | .. .. .. |
Notes. Columns 2–4 are for the first through third observations of each GC. For these columns, each one includes three numbers: the first number 
, 
is the width of the observed region (i.e., the angular distance over which the spectrograph slit is trailed, see Col. 5 of their Table 2), the second and third numbers, 
and 
, are for the length of the observed region and are displacements between the cluster center and the slit boundary (Col. 9 of their Table 2). The dots indicate that there is no corresponding observation.
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