Table 4.
Number counts (and fractions) of interlopers among the results of our first selection, for each NB.
Filters | First selection | SDSS spectra | GALEX | Gaia DR2 stars | LQAC QSOs | Multiple NB | Extended | Final [N; deg−2] |
---|---|---|---|---|---|---|---|---|
J0395 | 12 251 | 2192 (17.9%) | 2003 (16.4%) | 857 (7.0%) | 87 (0.7%) | 1312 (10.7%) | 6307 (51.5%) | 2547 ; 2.8 |
J0410 | 19 905 | 1983 (9.9%) | 2003 (10.1%) | 2738 (13.8%) | 56 (0.3%) | 1648 (8.3%) | 9557 (48.0%) | 5556 ; 6.2 |
J0430 | 24 813 | 2083 (8.4%) | 2597 (10.5%) | 2441 (9.8%) | 40 (0.2%) | 3313 (13.4%) | 15 468 (62.3%) | 4994 ; 5.6 |
J0515 | 15 213 | 523 (3.4%) | 1249 (8.2%) | 531 (3.5%) | 7 (0.05%) | 1282 (8.4%) | 12 992 (85.4%) | 1467 ; 1.5 |
Notes. We note that the extended fraction of our samples is particularly high for the J0515 NBs, suggesting that this filter is affected by a high level of contamination from extended low-z interlopers. Indeed, this is the only NB among the four that is susceptible to contamination from the strong [OIII] 4959 + 5007 doublet and H β line in addition to [NeIII] and [OII]. Sources with at least one identification as a secure interloper are excluded; the final number counts of Lyα-emitting candidates are shown in the last column on the right. The average sky density of these objects shows significant variation among the four lists, with an average of ∼4 deg−2 sources per filter. The complete catalogues of genuine candidates (i.e. after excluding securely identified interlopers) can be found at: https://www.j-plus.es/ancillarydata/dr1_lya_emitting_candidates.
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