Relative galaxy merger fractions and galaxy merger enhancement ratios as a function of galaxy overdensity.*
| |$\delta$| . | |$f_{\rm merger}^{\rm rel,cor}$| . | |$R_{\rm merger}$| . |
|---|---|---|
| (1) . | (2) . | (3) . |
| |$z\sim 2$| | ||
| 0.06 | |$0.200_{-0.004}^{+0.004}$| | |$1.000_{-0.016}^{+0.016}$| |
| 0.76 | |$0.206_{-0.009}^{+0.009}$| | |$1.023_{-0.034}^{+0.034}$| |
| |$z\sim 3$| | ||
| 0.06 | |$0.200_{-0.015}^{+0.015}$| | |$1.000_{-0.091}^{+0.091}$| |
| 0.94 | |$0.246_{-0.022}^{+0.025}$| | |$1.288_{-0.138}^{+0.153}$| |
| |$z\sim 4$|–5 | ||
| 0.22 | |$0.200_{-0.005}^{+0.005}$| | |$1.000_{-0.022}^{+0.022}$| |
| 2.64 | |$0.277_{-0.044}^{+0.052}$| | |$1.358_{-0.206}^{+0.240}$| |
| 5.11 | |$0.359_{-0.107}^{+0.142}$| | |$1.740_{-0.495}^{+0.661}$| |
| |$\delta$| . | |$f_{\rm merger}^{\rm rel,cor}$| . | |$R_{\rm merger}$| . |
|---|---|---|
| (1) . | (2) . | (3) . |
| |$z\sim 2$| | ||
| 0.06 | |$0.200_{-0.004}^{+0.004}$| | |$1.000_{-0.016}^{+0.016}$| |
| 0.76 | |$0.206_{-0.009}^{+0.009}$| | |$1.023_{-0.034}^{+0.034}$| |
| |$z\sim 3$| | ||
| 0.06 | |$0.200_{-0.015}^{+0.015}$| | |$1.000_{-0.091}^{+0.091}$| |
| 0.94 | |$0.246_{-0.022}^{+0.025}$| | |$1.288_{-0.138}^{+0.153}$| |
| |$z\sim 4$|–5 | ||
| 0.22 | |$0.200_{-0.005}^{+0.005}$| | |$1.000_{-0.022}^{+0.022}$| |
| 2.64 | |$0.277_{-0.044}^{+0.052}$| | |$1.358_{-0.206}^{+0.240}$| |
| 5.11 | |$0.359_{-0.107}^{+0.142}$| | |$1.740_{-0.495}^{+0.661}$| |
(1) Average values of galaxy overdensity in each |$\delta$| bin. (2) Relative galaxy merger fractions corrected for the chance projection effect. (3) Galaxy merger enhancement ratio, |$f_{\rm merger}^{\rm rel,cor}/f_{\rm merger}^{\rm rel,cor}(\delta \sim 0)$|.
Relative galaxy merger fractions and galaxy merger enhancement ratios as a function of galaxy overdensity.*
| |$\delta$| . | |$f_{\rm merger}^{\rm rel,cor}$| . | |$R_{\rm merger}$| . |
|---|---|---|
| (1) . | (2) . | (3) . |
| |$z\sim 2$| | ||
| 0.06 | |$0.200_{-0.004}^{+0.004}$| | |$1.000_{-0.016}^{+0.016}$| |
| 0.76 | |$0.206_{-0.009}^{+0.009}$| | |$1.023_{-0.034}^{+0.034}$| |
| |$z\sim 3$| | ||
| 0.06 | |$0.200_{-0.015}^{+0.015}$| | |$1.000_{-0.091}^{+0.091}$| |
| 0.94 | |$0.246_{-0.022}^{+0.025}$| | |$1.288_{-0.138}^{+0.153}$| |
| |$z\sim 4$|–5 | ||
| 0.22 | |$0.200_{-0.005}^{+0.005}$| | |$1.000_{-0.022}^{+0.022}$| |
| 2.64 | |$0.277_{-0.044}^{+0.052}$| | |$1.358_{-0.206}^{+0.240}$| |
| 5.11 | |$0.359_{-0.107}^{+0.142}$| | |$1.740_{-0.495}^{+0.661}$| |
| |$\delta$| . | |$f_{\rm merger}^{\rm rel,cor}$| . | |$R_{\rm merger}$| . |
|---|---|---|
| (1) . | (2) . | (3) . |
| |$z\sim 2$| | ||
| 0.06 | |$0.200_{-0.004}^{+0.004}$| | |$1.000_{-0.016}^{+0.016}$| |
| 0.76 | |$0.206_{-0.009}^{+0.009}$| | |$1.023_{-0.034}^{+0.034}$| |
| |$z\sim 3$| | ||
| 0.06 | |$0.200_{-0.015}^{+0.015}$| | |$1.000_{-0.091}^{+0.091}$| |
| 0.94 | |$0.246_{-0.022}^{+0.025}$| | |$1.288_{-0.138}^{+0.153}$| |
| |$z\sim 4$|–5 | ||
| 0.22 | |$0.200_{-0.005}^{+0.005}$| | |$1.000_{-0.022}^{+0.022}$| |
| 2.64 | |$0.277_{-0.044}^{+0.052}$| | |$1.358_{-0.206}^{+0.240}$| |
| 5.11 | |$0.359_{-0.107}^{+0.142}$| | |$1.740_{-0.495}^{+0.661}$| |
(1) Average values of galaxy overdensity in each |$\delta$| bin. (2) Relative galaxy merger fractions corrected for the chance projection effect. (3) Galaxy merger enhancement ratio, |$f_{\rm merger}^{\rm rel,cor}/f_{\rm merger}^{\rm rel,cor}(\delta \sim 0)$|.
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