Table 2.
Catalogs of spectroscopically confirmed protocluster members and member candidates used in this work.
| Reference | Selection method | Members |
|---|---|---|
| Spectroscopic | ||
| Pentericci et al. (2000) | Lyα emission | 15 |
| Kurk et al. (2004a) | Hα emission | 9 |
| Croft et al. (2005) | Lyα emission | 7 [17] |
| Doherty et al. (2010) | Hα emission | 2 [2] |
| Kuiper et al. (2011) | OII emission | 15 [1] |
| Tanaka et al. (2013) | OII/OIII emission | 4 [10] |
| Dannerbauer et al. (2014) | Specz | 11 [4] |
| Shimakawa et al. (2014) | Hα emission | 23 |
| Tadaki et al. (2019) | CO emission | 4 |
| Jin et al. (2021) | CO emission | 46 |
| Color or narrow-band selected | ||
| Pentericci et al. (2002) | photo-z | 3 |
| Kurk et al. (2004b) | Lyα emitter | 40 |
| Kurk et al. (2004b) | Hα emitter | 40 |
| Kurk et al. (2004b) | EROs | 44 |
| Dannerbauer et al. (2014) | FIR photo-z | 2 [4] |
| Shimakawa et al. (2018) | Hα emitter | 68 |
| Tadaki et al. (2019) | Hα emitter | 9 |
Notes. In the second column, we list the identification/selection method, while in the third column we report the number of confirmed or candidate members of the Spiderweb complex (2.0 < z < 2.3). Occasionally, the number of random sources in the Spiderweb field outside the range 2.0 < z < 2.3 is reported in square brackets. The catalogs were obtained independently in different works, but often overlap significantly because they are often derived from the same datasets. The total number of unique sources is 252. We find 161 sources with spectroscopic redshifts, of which 112 are in the range 2.0 < z < 2.3.
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