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Table 3.
Description of the selection criteria and sample properties in previous pair counts studies and in this work.
| Literature | Redshift range | Major/Minor separation | Δv | rp | Primary Galaxy Mass |
|---|---|---|---|---|---|
| [km s−1] | [kpc] | ||||
| (1) | (2) | (3) | (4) | (5) | (6) |
| de Ravel et al. (2009) | 0.5 < z < 0.9 | F1/F2 ≤ 4.0 | ≤500 | < 20 | log(M*/M⊙) ≥ 9.5 |
| Xu et al. (2012) | 0 ≤ z ≤ 0.6 | M1/M2 ≤ 2.5 | ≤500 (*) | 5 − 20 | 9.8 < log(M*/M⊙) ≤ 10.2 |
| López-Sanjuan et al. (2013) | 0.9 < z < 1.8 | F1/F2 ≤ 4.0 | ≤500 | < 20 | 9 < log(M*/M⊙)< 11 |
| Tasca et al. (2014) | 1.8 ≤ z ≤ 4.0 | M1/M2 ≤ 4.0 | ≤500 | < 25 | 9 < log(M*/M⊙)< 11 |
| Ventou et al. (2017) | 0.2 ≤ z ≤ 4.0 | M1/M2 ≤ 6.0 | ≤500 | < 25 | log(M*/M⊙) ≥ 9.5 |
| Duncan et al. (2019) | 0.5 ≤ z < 3.5 | M1/M2 ≤ 4.0 | ≤500 (*) | 5 − 30 | 9.7 < log(M*/M⊙)< 10.3 |
| This work | 4.4 ≤ z < 5.9 | M1/M2 ≤ 4.0 | ≤500 | < 20 | 9 ≲ log(M*/M⊙) ≲ 11 |
Notes. The asterisks in Col. 4 indicate the works in the literature that made use of photometric redshifts to define the selection criterion on the velocity separation between pairs.
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