Estimated average galaxy properties based on the photometric and spectroscopic stacking. The values in the parenthesis correspond to the 1σ uncertainty. Line luminosities are measured in the units of |$10^{40}\, \rm {erg\, s^{-1}}$|.
Redshift . | Sample . | mg . | mr . | mz . | |$L_{[{\rm O\, \small {\rm II}}]}$| . | LHβ . | |$L_{[{\rm O\, \small {\rm III}}]}$| . | |$L_{[{\rm O\, \small {\rm III}}]}$| . |
---|---|---|---|---|---|---|---|---|
. | . | . | . | . | λ3728 . | λ4862 . | λ4960 . | λ5008 . |
0.35–0.625 | All | |$22.97^{+0.56}_{-0.89}$| | |$21.80^{+0.23}_{-0.26}$| | |$22.16^{+0.48}_{-0.65}$| | 9.98(0.32) | 3.48(0.25) | 2.57(0.27) | 6.93(0.25) |
(low-z) | GOTOQ-Ext | |$22.63^{+0.85}_{-0.95}$| | |$21.43^{+0.40}_{-0.68}$| | |$21.04^{+0.26}_{-0.37}$| | 11.2(0.5) | 4.0(0.4) | 2.9(0.4) | 11.0(0.5) |
GOTOQ-Noext | |$22.90^{+0.65}_{-0.97}$| | |$22.32^{+0.31}_{-0.82}$| | |$22.11^{+0.39}_{-0.71}$| | 9.7(0.4) | 2.96(0.31) | 2.75(0.31) | 5.70(0.31) | |
0.625–0.748 | All | |$23.39^{+0.59}_{-0.85}$| | |$22.37^{+0.35}_{-0.58}$| | |$22.89^{+0.44}_{-0.93}$| | 18.9(0.7) | 3.8(0.6) | 4.2(0.9) | 10.9(0.8) |
(mid-z) | GOTOQ-Ext | |$22.38^{+0.73}_{-1.03}$| | |$22.27^{+0.58}_{-0.95}$| | |$22.81^{+0.53}_{-0.83}$| | 19.8(0.8) | 4.3(0.9) | 5.7(1.2) | 11.9(1.2) |
GOTOQ-Noext | |$22.63^{+0.97}_{-0.60}$| | |$22.34^{+0.62}_{-0.68}$| | |$22.49^{+0.70}_{-0.70}$| | 19.7(1.0) | ≤2.7 | 4.3(1.3) | 10.6(1.4) | |
0.748–1.06 | All | |$24.00^{^+0.59}_{-1.10}$| | |$22.78^{+0.51}_{-0.70}$| | |$23.07^{+0.52}_{-1.12}$| | 25.5(0.8) | 9.5(1.3) | ≤7.2 | 22.4(2.4) |
(high-z) |
Redshift . | Sample . | mg . | mr . | mz . | |$L_{[{\rm O\, \small {\rm II}}]}$| . | LHβ . | |$L_{[{\rm O\, \small {\rm III}}]}$| . | |$L_{[{\rm O\, \small {\rm III}}]}$| . |
---|---|---|---|---|---|---|---|---|
. | . | . | . | . | λ3728 . | λ4862 . | λ4960 . | λ5008 . |
0.35–0.625 | All | |$22.97^{+0.56}_{-0.89}$| | |$21.80^{+0.23}_{-0.26}$| | |$22.16^{+0.48}_{-0.65}$| | 9.98(0.32) | 3.48(0.25) | 2.57(0.27) | 6.93(0.25) |
(low-z) | GOTOQ-Ext | |$22.63^{+0.85}_{-0.95}$| | |$21.43^{+0.40}_{-0.68}$| | |$21.04^{+0.26}_{-0.37}$| | 11.2(0.5) | 4.0(0.4) | 2.9(0.4) | 11.0(0.5) |
GOTOQ-Noext | |$22.90^{+0.65}_{-0.97}$| | |$22.32^{+0.31}_{-0.82}$| | |$22.11^{+0.39}_{-0.71}$| | 9.7(0.4) | 2.96(0.31) | 2.75(0.31) | 5.70(0.31) | |
0.625–0.748 | All | |$23.39^{+0.59}_{-0.85}$| | |$22.37^{+0.35}_{-0.58}$| | |$22.89^{+0.44}_{-0.93}$| | 18.9(0.7) | 3.8(0.6) | 4.2(0.9) | 10.9(0.8) |
(mid-z) | GOTOQ-Ext | |$22.38^{+0.73}_{-1.03}$| | |$22.27^{+0.58}_{-0.95}$| | |$22.81^{+0.53}_{-0.83}$| | 19.8(0.8) | 4.3(0.9) | 5.7(1.2) | 11.9(1.2) |
GOTOQ-Noext | |$22.63^{+0.97}_{-0.60}$| | |$22.34^{+0.62}_{-0.68}$| | |$22.49^{+0.70}_{-0.70}$| | 19.7(1.0) | ≤2.7 | 4.3(1.3) | 10.6(1.4) | |
0.748–1.06 | All | |$24.00^{^+0.59}_{-1.10}$| | |$22.78^{+0.51}_{-0.70}$| | |$23.07^{+0.52}_{-1.12}$| | 25.5(0.8) | 9.5(1.3) | ≤7.2 | 22.4(2.4) |
(high-z) |
Estimated average galaxy properties based on the photometric and spectroscopic stacking. The values in the parenthesis correspond to the 1σ uncertainty. Line luminosities are measured in the units of |$10^{40}\, \rm {erg\, s^{-1}}$|.
Redshift . | Sample . | mg . | mr . | mz . | |$L_{[{\rm O\, \small {\rm II}}]}$| . | LHβ . | |$L_{[{\rm O\, \small {\rm III}}]}$| . | |$L_{[{\rm O\, \small {\rm III}}]}$| . |
---|---|---|---|---|---|---|---|---|
. | . | . | . | . | λ3728 . | λ4862 . | λ4960 . | λ5008 . |
0.35–0.625 | All | |$22.97^{+0.56}_{-0.89}$| | |$21.80^{+0.23}_{-0.26}$| | |$22.16^{+0.48}_{-0.65}$| | 9.98(0.32) | 3.48(0.25) | 2.57(0.27) | 6.93(0.25) |
(low-z) | GOTOQ-Ext | |$22.63^{+0.85}_{-0.95}$| | |$21.43^{+0.40}_{-0.68}$| | |$21.04^{+0.26}_{-0.37}$| | 11.2(0.5) | 4.0(0.4) | 2.9(0.4) | 11.0(0.5) |
GOTOQ-Noext | |$22.90^{+0.65}_{-0.97}$| | |$22.32^{+0.31}_{-0.82}$| | |$22.11^{+0.39}_{-0.71}$| | 9.7(0.4) | 2.96(0.31) | 2.75(0.31) | 5.70(0.31) | |
0.625–0.748 | All | |$23.39^{+0.59}_{-0.85}$| | |$22.37^{+0.35}_{-0.58}$| | |$22.89^{+0.44}_{-0.93}$| | 18.9(0.7) | 3.8(0.6) | 4.2(0.9) | 10.9(0.8) |
(mid-z) | GOTOQ-Ext | |$22.38^{+0.73}_{-1.03}$| | |$22.27^{+0.58}_{-0.95}$| | |$22.81^{+0.53}_{-0.83}$| | 19.8(0.8) | 4.3(0.9) | 5.7(1.2) | 11.9(1.2) |
GOTOQ-Noext | |$22.63^{+0.97}_{-0.60}$| | |$22.34^{+0.62}_{-0.68}$| | |$22.49^{+0.70}_{-0.70}$| | 19.7(1.0) | ≤2.7 | 4.3(1.3) | 10.6(1.4) | |
0.748–1.06 | All | |$24.00^{^+0.59}_{-1.10}$| | |$22.78^{+0.51}_{-0.70}$| | |$23.07^{+0.52}_{-1.12}$| | 25.5(0.8) | 9.5(1.3) | ≤7.2 | 22.4(2.4) |
(high-z) |
Redshift . | Sample . | mg . | mr . | mz . | |$L_{[{\rm O\, \small {\rm II}}]}$| . | LHβ . | |$L_{[{\rm O\, \small {\rm III}}]}$| . | |$L_{[{\rm O\, \small {\rm III}}]}$| . |
---|---|---|---|---|---|---|---|---|
. | . | . | . | . | λ3728 . | λ4862 . | λ4960 . | λ5008 . |
0.35–0.625 | All | |$22.97^{+0.56}_{-0.89}$| | |$21.80^{+0.23}_{-0.26}$| | |$22.16^{+0.48}_{-0.65}$| | 9.98(0.32) | 3.48(0.25) | 2.57(0.27) | 6.93(0.25) |
(low-z) | GOTOQ-Ext | |$22.63^{+0.85}_{-0.95}$| | |$21.43^{+0.40}_{-0.68}$| | |$21.04^{+0.26}_{-0.37}$| | 11.2(0.5) | 4.0(0.4) | 2.9(0.4) | 11.0(0.5) |
GOTOQ-Noext | |$22.90^{+0.65}_{-0.97}$| | |$22.32^{+0.31}_{-0.82}$| | |$22.11^{+0.39}_{-0.71}$| | 9.7(0.4) | 2.96(0.31) | 2.75(0.31) | 5.70(0.31) | |
0.625–0.748 | All | |$23.39^{+0.59}_{-0.85}$| | |$22.37^{+0.35}_{-0.58}$| | |$22.89^{+0.44}_{-0.93}$| | 18.9(0.7) | 3.8(0.6) | 4.2(0.9) | 10.9(0.8) |
(mid-z) | GOTOQ-Ext | |$22.38^{+0.73}_{-1.03}$| | |$22.27^{+0.58}_{-0.95}$| | |$22.81^{+0.53}_{-0.83}$| | 19.8(0.8) | 4.3(0.9) | 5.7(1.2) | 11.9(1.2) |
GOTOQ-Noext | |$22.63^{+0.97}_{-0.60}$| | |$22.34^{+0.62}_{-0.68}$| | |$22.49^{+0.70}_{-0.70}$| | 19.7(1.0) | ≤2.7 | 4.3(1.3) | 10.6(1.4) | |
0.748–1.06 | All | |$24.00^{^+0.59}_{-1.10}$| | |$22.78^{+0.51}_{-0.70}$| | |$23.07^{+0.52}_{-1.12}$| | 25.5(0.8) | 9.5(1.3) | ≤7.2 | 22.4(2.4) |
(high-z) |
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