Table 2.

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)NσtotσmeasσintNσtotσmeasσintNσtotσmeasσintNσtotσmeasσint
4.9(z = 0.48)2260.360.080.354270.320.070.323430.390.060.3940
6.1(z = 0.66)2220.310.090.295320.320.080.316740.380.070.371950.480.080.47
7.3(z = 0.90)2400.280.110.266480.320.090.3110820.350.090.335040.400.070.39
8.5(z = 1.22)2190.340.110.326960.330.100.3111280.300.090.287580.380.090.37
9.7(z = 1.70)2800.280.090.278550.290.090.2716070.320.080.3113160.320.080.31
10.9(z = 2.51)491310.260.070.251400.350.090.341570.290.100.27
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)NσtotσmeasσintNσtotσmeasσintNσtotσmeasσintNσtotσmeasσint
4.9(z = 0.48)2260.360.080.354270.320.070.323430.390.060.3940
6.1(z = 0.66)2220.310.090.295320.320.080.316740.380.070.371950.480.080.47
7.3(z = 0.90)2400.280.110.266480.320.090.3110820.350.090.335040.400.070.39
8.5(z = 1.22)2190.340.110.326960.330.100.3111280.300.090.287580.380.090.37
9.7(z = 1.70)2800.280.090.278550.290.090.2716070.320.080.3113160.320.080.31
10.9(z = 2.51)491310.260.070.251400.350.090.341570.290.100.27
Table 2.

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)NσtotσmeasσintNσtotσmeasσintNσtotσmeasσintNσtotσmeasσint
4.9(z = 0.48)2260.360.080.354270.320.070.323430.390.060.3940
6.1(z = 0.66)2220.310.090.295320.320.080.316740.380.070.371950.480.080.47
7.3(z = 0.90)2400.280.110.266480.320.090.3110820.350.090.335040.400.070.39
8.5(z = 1.22)2190.340.110.326960.330.100.3111280.300.090.287580.380.090.37
9.7(z = 1.70)2800.280.090.278550.290.090.2716070.320.080.3113160.320.080.31
10.9(z = 2.51)491310.260.070.251400.350.090.341570.290.100.27
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)NσtotσmeasσintNσtotσmeasσintNσtotσmeasσintNσtotσmeasσint
4.9(z = 0.48)2260.360.080.354270.320.070.323430.390.060.3940
6.1(z = 0.66)2220.310.090.295320.320.080.316740.380.070.371950.480.080.47
7.3(z = 0.90)2400.280.110.266480.320.090.3110820.350.090.335040.400.070.39
8.5(z = 1.22)2190.340.110.326960.330.100.3111280.300.090.287580.380.090.37
9.7(z = 1.70)2800.280.090.278550.290.090.2716070.320.080.3113160.320.080.31
10.9(z = 2.51)491310.260.070.251400.350.090.341570.290.100.27
Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close