Look-back time version of Table 1 by collecting and reassigning the 12 380 mass-complete data to six tlb bins. We exclude bins in which the number of galaxies is less than 50 (>1011 M⊙ at tlb = 4.9 Gyr), together with the mass-incomplete data. In general, the intrinsic MS scatter is still significantly larger than measurement uncertainty in new binning criteria, which avoids the effect of non-linear tlb widths in previous zphot binning.
M* . | |$9.5\!-\!10.0\log({\rm M}_{\odot }$|) . | |$10.0\!-\!10.5\log({\rm M}_{\odot }$|) . | |$10.5\!-\!11.0\log({\rm M}_{\odot })$| . | |$\gt 11.0\log({\rm M}_{\odot }$|) . | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
tlb(Gyr) . | N . | σtot . | σmeas . | σint . | N . | σtot . | σmeas . | σint . | N . | σtot . | σmeas . | σint . | N . | σtot . | σmeas . | σint . |
4.9(z = 0.48) | 226 | 0.36 | 0.08 | 0.35 | 427 | 0.32 | 0.07 | 0.32 | 343 | 0.39 | 0.06 | 0.39 | 40 | – | – | – |
6.1(z = 0.66) | 222 | 0.31 | 0.09 | 0.29 | 532 | 0.32 | 0.08 | 0.31 | 674 | 0.38 | 0.07 | 0.37 | 195 | 0.48 | 0.08 | 0.47 |
7.3(z = 0.90) | 240 | 0.28 | 0.11 | 0.26 | 648 | 0.32 | 0.09 | 0.31 | 1082 | 0.35 | 0.09 | 0.33 | 504 | 0.40 | 0.07 | 0.39 |
8.5(z = 1.22) | 219 | 0.34 | 0.11 | 0.32 | 696 | 0.33 | 0.10 | 0.31 | 1128 | 0.30 | 0.09 | 0.28 | 758 | 0.38 | 0.09 | 0.37 |
9.7(z = 1.70) | 280 | 0.28 | 0.09 | 0.27 | 855 | 0.29 | 0.09 | 0.27 | 1607 | 0.32 | 0.08 | 0.31 | 1316 | 0.32 | 0.08 | 0.31 |
10.9(z = 2.51) | 49 | – | – | – | 131 | 0.26 | 0.07 | 0.25 | 140 | 0.35 | 0.09 | 0.34 | 157 | 0.29 | 0.10 | 0.27 |
M* . | |$9.5\!-\!10.0\log({\rm M}_{\odot }$|) . | |$10.0\!-\!10.5\log({\rm M}_{\odot }$|) . | |$10.5\!-\!11.0\log({\rm M}_{\odot })$| . | |$\gt 11.0\log({\rm M}_{\odot }$|) . | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
tlb(Gyr) . | N . | σtot . | σmeas . | σint . | N . | σtot . | σmeas . | σint . | N . | σtot . | σmeas . | σint . | N . | σtot . | σmeas . | σint . |
4.9(z = 0.48) | 226 | 0.36 | 0.08 | 0.35 | 427 | 0.32 | 0.07 | 0.32 | 343 | 0.39 | 0.06 | 0.39 | 40 | – | – | – |
6.1(z = 0.66) | 222 | 0.31 | 0.09 | 0.29 | 532 | 0.32 | 0.08 | 0.31 | 674 | 0.38 | 0.07 | 0.37 | 195 | 0.48 | 0.08 | 0.47 |
7.3(z = 0.90) | 240 | 0.28 | 0.11 | 0.26 | 648 | 0.32 | 0.09 | 0.31 | 1082 | 0.35 | 0.09 | 0.33 | 504 | 0.40 | 0.07 | 0.39 |
8.5(z = 1.22) | 219 | 0.34 | 0.11 | 0.32 | 696 | 0.33 | 0.10 | 0.31 | 1128 | 0.30 | 0.09 | 0.28 | 758 | 0.38 | 0.09 | 0.37 |
9.7(z = 1.70) | 280 | 0.28 | 0.09 | 0.27 | 855 | 0.29 | 0.09 | 0.27 | 1607 | 0.32 | 0.08 | 0.31 | 1316 | 0.32 | 0.08 | 0.31 |
10.9(z = 2.51) | 49 | – | – | – | 131 | 0.26 | 0.07 | 0.25 | 140 | 0.35 | 0.09 | 0.34 | 157 | 0.29 | 0.10 | 0.27 |
Look-back time version of Table 1 by collecting and reassigning the 12 380 mass-complete data to six tlb bins. We exclude bins in which the number of galaxies is less than 50 (>1011 M⊙ at tlb = 4.9 Gyr), together with the mass-incomplete data. In general, the intrinsic MS scatter is still significantly larger than measurement uncertainty in new binning criteria, which avoids the effect of non-linear tlb widths in previous zphot binning.
M* . | |$9.5\!-\!10.0\log({\rm M}_{\odot }$|) . | |$10.0\!-\!10.5\log({\rm M}_{\odot }$|) . | |$10.5\!-\!11.0\log({\rm M}_{\odot })$| . | |$\gt 11.0\log({\rm M}_{\odot }$|) . | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
tlb(Gyr) . | N . | σtot . | σmeas . | σint . | N . | σtot . | σmeas . | σint . | N . | σtot . | σmeas . | σint . | N . | σtot . | σmeas . | σint . |
4.9(z = 0.48) | 226 | 0.36 | 0.08 | 0.35 | 427 | 0.32 | 0.07 | 0.32 | 343 | 0.39 | 0.06 | 0.39 | 40 | – | – | – |
6.1(z = 0.66) | 222 | 0.31 | 0.09 | 0.29 | 532 | 0.32 | 0.08 | 0.31 | 674 | 0.38 | 0.07 | 0.37 | 195 | 0.48 | 0.08 | 0.47 |
7.3(z = 0.90) | 240 | 0.28 | 0.11 | 0.26 | 648 | 0.32 | 0.09 | 0.31 | 1082 | 0.35 | 0.09 | 0.33 | 504 | 0.40 | 0.07 | 0.39 |
8.5(z = 1.22) | 219 | 0.34 | 0.11 | 0.32 | 696 | 0.33 | 0.10 | 0.31 | 1128 | 0.30 | 0.09 | 0.28 | 758 | 0.38 | 0.09 | 0.37 |
9.7(z = 1.70) | 280 | 0.28 | 0.09 | 0.27 | 855 | 0.29 | 0.09 | 0.27 | 1607 | 0.32 | 0.08 | 0.31 | 1316 | 0.32 | 0.08 | 0.31 |
10.9(z = 2.51) | 49 | – | – | – | 131 | 0.26 | 0.07 | 0.25 | 140 | 0.35 | 0.09 | 0.34 | 157 | 0.29 | 0.10 | 0.27 |
M* . | |$9.5\!-\!10.0\log({\rm M}_{\odot }$|) . | |$10.0\!-\!10.5\log({\rm M}_{\odot }$|) . | |$10.5\!-\!11.0\log({\rm M}_{\odot })$| . | |$\gt 11.0\log({\rm M}_{\odot }$|) . | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
tlb(Gyr) . | N . | σtot . | σmeas . | σint . | N . | σtot . | σmeas . | σint . | N . | σtot . | σmeas . | σint . | N . | σtot . | σmeas . | σint . |
4.9(z = 0.48) | 226 | 0.36 | 0.08 | 0.35 | 427 | 0.32 | 0.07 | 0.32 | 343 | 0.39 | 0.06 | 0.39 | 40 | – | – | – |
6.1(z = 0.66) | 222 | 0.31 | 0.09 | 0.29 | 532 | 0.32 | 0.08 | 0.31 | 674 | 0.38 | 0.07 | 0.37 | 195 | 0.48 | 0.08 | 0.47 |
7.3(z = 0.90) | 240 | 0.28 | 0.11 | 0.26 | 648 | 0.32 | 0.09 | 0.31 | 1082 | 0.35 | 0.09 | 0.33 | 504 | 0.40 | 0.07 | 0.39 |
8.5(z = 1.22) | 219 | 0.34 | 0.11 | 0.32 | 696 | 0.33 | 0.10 | 0.31 | 1128 | 0.30 | 0.09 | 0.28 | 758 | 0.38 | 0.09 | 0.37 |
9.7(z = 1.70) | 280 | 0.28 | 0.09 | 0.27 | 855 | 0.29 | 0.09 | 0.27 | 1607 | 0.32 | 0.08 | 0.31 | 1316 | 0.32 | 0.08 | 0.31 |
10.9(z = 2.51) | 49 | – | – | – | 131 | 0.26 | 0.07 | 0.25 | 140 | 0.35 | 0.09 | 0.34 | 157 | 0.29 | 0.10 | 0.27 |
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