Table 2.

Properties of the colour-selected samples. ‘b’ stands for bright (20 < g < 22.5 for ugr or 19 < i < 21.3 for gri) and ‘f’ stands for faint (22.5 < g < 23.5 for ugr or 21.3 < i < 23 for gri). We indicate the mean and standard deviation of the redshift distribution for each set. For the CMC sample, [O ii] fluxes are expressed in units of 10−17 erg cm−2 s−1; the median, the first and third quartiles of the flux distribution are indicated. The ugr tends to select the highest [O ii] fluxes.

SelectionNo.deg− 2|$\bar{u}$||$\bar{g}$||$\bar{r}$||$\bar{i}$||$\bar{z}$|σz|$\bar{f}_{\left[\mathrm{O\,{\rm II}}\right]}$||$Q^1_{f_{\left[\mathrm{O\,{\rm II}}\right]}}$||$Q^3_{f_{\left[\mathrm{O\,{\rm II}}\right]}}$|
CMCugrb130.021.9821.8721.691.250.5361.7446.4788.39
f1450.823.2723.1822.981.190.3816.6013.0622.26
grib257.222.6921.8720.930.800.2113.858.6522.21
f2170.523.3423.0922.550.930.3110.236.8315.99
CFHT-W1ugrb193.321.9521.821.71.280.38
f1766.823.3723.1923.071.290.31
grib361.422.6221.820.820.810.11
f3317.523.3423.1122.551.030.35
CFHT-W3ugrb232.221.8921.7621.691.270.37
f1679.123.3623.1823.061.280.31
grib391.622.6221.7820.80.820.1
f3334.223.3423.1122.541.030.33
SDSSugrb166.9621.7621.7721.52
grib204.9622.5721.7520.76
SelectionNo.deg− 2|$\bar{u}$||$\bar{g}$||$\bar{r}$||$\bar{i}$||$\bar{z}$|σz|$\bar{f}_{\left[\mathrm{O\,{\rm II}}\right]}$||$Q^1_{f_{\left[\mathrm{O\,{\rm II}}\right]}}$||$Q^3_{f_{\left[\mathrm{O\,{\rm II}}\right]}}$|
CMCugrb130.021.9821.8721.691.250.5361.7446.4788.39
f1450.823.2723.1822.981.190.3816.6013.0622.26
grib257.222.6921.8720.930.800.2113.858.6522.21
f2170.523.3423.0922.550.930.3110.236.8315.99
CFHT-W1ugrb193.321.9521.821.71.280.38
f1766.823.3723.1923.071.290.31
grib361.422.6221.820.820.810.11
f3317.523.3423.1122.551.030.35
CFHT-W3ugrb232.221.8921.7621.691.270.37
f1679.123.3623.1823.061.280.31
grib391.622.6221.7820.80.820.1
f3334.223.3423.1122.541.030.33
SDSSugrb166.9621.7621.7721.52
grib204.9622.5721.7520.76
Table 2.

Properties of the colour-selected samples. ‘b’ stands for bright (20 < g < 22.5 for ugr or 19 < i < 21.3 for gri) and ‘f’ stands for faint (22.5 < g < 23.5 for ugr or 21.3 < i < 23 for gri). We indicate the mean and standard deviation of the redshift distribution for each set. For the CMC sample, [O ii] fluxes are expressed in units of 10−17 erg cm−2 s−1; the median, the first and third quartiles of the flux distribution are indicated. The ugr tends to select the highest [O ii] fluxes.

SelectionNo.deg− 2|$\bar{u}$||$\bar{g}$||$\bar{r}$||$\bar{i}$||$\bar{z}$|σz|$\bar{f}_{\left[\mathrm{O\,{\rm II}}\right]}$||$Q^1_{f_{\left[\mathrm{O\,{\rm II}}\right]}}$||$Q^3_{f_{\left[\mathrm{O\,{\rm II}}\right]}}$|
CMCugrb130.021.9821.8721.691.250.5361.7446.4788.39
f1450.823.2723.1822.981.190.3816.6013.0622.26
grib257.222.6921.8720.930.800.2113.858.6522.21
f2170.523.3423.0922.550.930.3110.236.8315.99
CFHT-W1ugrb193.321.9521.821.71.280.38
f1766.823.3723.1923.071.290.31
grib361.422.6221.820.820.810.11
f3317.523.3423.1122.551.030.35
CFHT-W3ugrb232.221.8921.7621.691.270.37
f1679.123.3623.1823.061.280.31
grib391.622.6221.7820.80.820.1
f3334.223.3423.1122.541.030.33
SDSSugrb166.9621.7621.7721.52
grib204.9622.5721.7520.76
SelectionNo.deg− 2|$\bar{u}$||$\bar{g}$||$\bar{r}$||$\bar{i}$||$\bar{z}$|σz|$\bar{f}_{\left[\mathrm{O\,{\rm II}}\right]}$||$Q^1_{f_{\left[\mathrm{O\,{\rm II}}\right]}}$||$Q^3_{f_{\left[\mathrm{O\,{\rm II}}\right]}}$|
CMCugrb130.021.9821.8721.691.250.5361.7446.4788.39
f1450.823.2723.1822.981.190.3816.6013.0622.26
grib257.222.6921.8720.930.800.2113.858.6522.21
f2170.523.3423.0922.550.930.3110.236.8315.99
CFHT-W1ugrb193.321.9521.821.71.280.38
f1766.823.3723.1923.071.290.31
grib361.422.6221.820.820.810.11
f3317.523.3423.1122.551.030.35
CFHT-W3ugrb232.221.8921.7621.691.270.37
f1679.123.3623.1823.061.280.31
grib391.622.6221.7820.80.820.1
f3334.223.3423.1122.541.030.33
SDSSugrb166.9621.7621.7721.52
grib204.9622.5721.7520.76
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