Table A.1.
Unclear merged detections.
| Apertif name | Nsample | reason |
|---|---|---|
| AHC- | ||
| J120231.7+614724 | 2 | res |
| J123353.2+393735 | 2 | res |
| J131401.5+552253 | 2 | res |
| J222934.9+511016 | 2 | res |
| J235942.6+342048 | 2 | res |
| J120107.6+544859 | 2 | res&snr |
| J232356.9+481659 | 1 | res&snr |
| J024158.7+410448 | 2 | snr&uoc |
| J143904.6+380854 | 1 | snr&uoc |
Notes. The Apertif name is based on the detection position, using the right ascension and declination in J2000 as: AHCJhhmmss.s+ddmmss. Nsample denotes the number of galaxies in the detection that entered our parent dwarf sample. All unclear detections are thought to contain at most two galaxies. The reason explains why the detection was classified as unclear. Possibilities include: res - insufficient spatial resolution of the H I emission; snr - too low S/N of the H I detection; uoc - unclear optical counterpart; or a combination of these.
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