Table C.1
Integrated number of Hα emitters expected in the UltraVISTA survey above different flux thresholds.
| Flux [10-17 ergs-1cm-2] | |||||
| LF | all | >3.0 | >5.0 | >10.0 | >20.0 |
|
|
|||||
| UltraVISTA DR2a,c | |||||
|
|
|||||
| LY11 | 184 (113) | 169 (113) | 119 (90) | 77 (60) | 39 (30) |
| SO09 | 250 (165) | 237 (164) | 184 (140) | 132 (102) | 76 (59) |
| VI08 | 275 (156) | 246 (155) | 150 (113) | 79 (61) | 25 (19) |
|
|
|||||
| Full UltraVISTAb,c | |||||
|
|
|||||
| LY11 | 373 (235) | 198 (154) | 126 (98) | 79 (62) | 39 (30) |
| SO09 | 413 (280) | 268 (209) | 192 (150) | 135 (106) | 76 (60) |
| VI08 | 666 (400) | 299 (233) | 161 (126) | 81 (64) | 25 (19) |
Notes. For more details see caption of Fig. C.1.
Values outside the parentheses are for w6583 = 0.3 and inside parentheses for w6583 = 0. The numbers are for those parts of the field with coverage in two different NB118 filters.
Reference. Ly et al. (2011, LY11); Sobral et al. (2009, S09); Villar et al. (2008, VI08).
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