Table E.1.
Comparison between the detection statistics across different SBe bins.
| SBe | Input dwarfs | In MER catalogue | Single parent ID |
|---|---|---|---|
| (1) | (2) | (3) | (4) |
| 21–22 | 6 (100 %) | 2 (33 %) | 6 (100 %) |
| 22–23 | 18 (100 %) | 8 (44 %) | 14 (78 %) |
| 23–24 | 68 (100 %) | 51 (75 %) | 64 (94 %) |
| 24–25 | 192 (100 %) | 123 (64 %) | 154 (80 %) |
| 25–26 | 202 (100%) | 104 (51%) | 114 (56 %) |
| 26–27 | 173 (100 %) | 28 (16%) | 54 (31 %) |
| 27–28 | 101 (100 %) | 17 (17%) | 38 (38 %) |
| 28–29 | 11 (100 %) | 3 (27 %) | 7 (63 %) |
| 29–30 | 16 (100 %) | 4 (25 %) | 8 (50 %) |
| 30–31 | 4 (100 %) | 1 (25 %) | 1 (25 %) |
Notes. Column (1) gives the SBe bin in mag arcsec−2. Columns (2) indicates the number of injected dwarfs. The remaining columns are the number of dwarfs that are (3) present in the final MER catalogue as one single object, (4) present in the final MER catalogue as one or several objects sharing the same parent ID. Column (4) includes the detections from Column (3). They are given in number and in percent of the injected dwarfs in the corresponding surface brightness bin.
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