| EW0 |  |
 |
# | #H | n1138 | n |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
| 50 | 3 | - | 17 | 2 |  |
|
| 25 | 3 | - | 23 | 3 |  |
|
| 25 | 2 | - | 40 | 3 |  |
|
| 50 | 1 | - | 48 | 2 |  |
|
| 25 | 1 | - | 60 | 3 |  |
|
| 75 | 2 | 19.3 | 1 | 0 |  |
 |
| 100 | 3 | 19.5 | 2 | 1 |  |
 |
Notes: (1) Rest frame equivalent width lower
limit; (2) signal to noise lower limit as defined by Bunker et al. (1995);
(3) additional selection criterion: narrow band magnitude upper limit;
(4) number of candidates in 12.5 arcmin2 area; (5) number of
candidates within the radio galaxy Ly
halo; (6) surface density of
candidates in the field of 1138-262 (arcmin-2); (7) surface density
in other fields: a Bunker et al. (1995), b van der Werf et al. (2000).
|