Table 3.
Statistics for each class of objects as a function of redshift confidence level (CONFID) in the MAGIC survey.
| Class | CONFID |
||||
|---|---|---|---|---|---|
| 1 | 2 | 3 | 1–3 | ||
| Stars | 16 (0) | 7 (0) | 37 (0) | 60 (0) | 4% |
| Nearby | 2 (0) | 10 (1) | 30 (3) | 42 (4) | 2% |
| [O II] | 100 (9) | 500 (60) | 654 (46) | 1254 (115) | 75% |
| Desert | 43 (4) | 34 (3) | 7 (1) | 84 (8) | 5% |
| Lyα | 103 (26) | 109 (48) | 31 (10) | 243 (84) | 14% |
| All | 264 (39) | 660 (112) | 759 (60) | 1683 (211) | 100% |
Notes. The first four columns indicate the number of objects, whereas the last column indicates the fraction of objects for each class. All sources are included, except those having defects (usually at the edge of MUSE fields) with CONFID equal to unity. Numbers into parentheses correspond to sources found from blind search and deblending. Stars all have z < 0.0005, nearby galaxies have 0.0005 ≤ z < 0.25, potential [O II] emitters have 0.25 ≤ z < 1.5, redshift desert corresponds to 1.5 ≤ z < 2.9 and potential Lyα emitters have z ≥ 2.9.
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