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Table 4:

Best fitting parameters for the MIPS-d sample.
ID $z_{\rm phot}$ $\chi ^2_{\nu }$ $P_{\chi^2_{\nu}}$ AV $z_{{\rm inf}-90\%}$ $z_{{\rm sup}-90\%}$ $z_{\rm 2-phot}$ $P_{\chi^2_{\nu},2}$ log M
#588 4.285 0.785 64.36 0.60 3.690 4.740 9.388 0.05 9.973
#702 8.814 0.067 99.99 0.40 1.450 10.060 3.340 99.99 10.563
#1720 3.522 0.526 87.33 0.60 2.850 4.250 3.921 84.30 10.399
#2172 3.711 0.536 86.56 0.70 3.550 4.180 4.117 70.42 11.097
#2560 3.830 0.044 100.00 0.40 2.780 8.520 7.274 100.00 10.762
#2796 10.060 0.279 98.59 0.80 3.360 10.060 3.536 95.36 10.870a
#2894 3.893 0.628 79.14 0.70 2.990 4.460 10.060 0.37 10.441
#3393 5.503 0.477 90.59 0.80 3.830 5.860 5.167 84.73 10.647
#3850 4.166 0.063 100.00 0.70 3.410 9.290 8.009 99.90 10.940
#5157 4.740 0.344 96.90 0.00 4.110 7.400 6.504 92.59 11.433
#5367 4.355 0.494 89.51 0.80 3.900 4.880 10.060 0.03 10.806
#5511 4.152 2.521 0.50 0.50 4.040 4.250 1.310 0.00 10.551
#6099 5.251 0.367 96.10 0.10 3.200 8.450 4.999 96.02 11.178
#6245 5.062 0.108 99.98 0.00 4.460 5.370 2.934 81.31 10.662
#6463 9.437 0.193 99.68 0.10 3.690 10.060 4.215 99.64 9.973a
#8520 3.683 0.573 83.71 0.00 3.340 3.830 3.137 44.99 10.730
#9007 3.669 1.117 34.42 0.60 2.780 4.110 2.969 34.41 10.824
#9301 8.226 0.059 100.00 0.20 2.640 10.060 8.037 100.00 11.035
#9306 8.660 0.127 99.95 0.80 2.360 10.060 8.219 99.92 11.011
#9782 3.928 1.472 14.28 0.20 3.480 4.320 8.723 0.02 11.116
#10176 5.818 0.002 100.00 0.20 3.550 9.570 5.517 100.00 11.280
#11304 4.145 0.378 95.67 0.80 3.550 8.100 5.461 89.78 10.759
#12699 3.543 1.760 6.21 0.30 3.200 3.690 3.354 5.62 10.558
#13129 7.960 0.030 100.00 0.20 3.410 10.060 8.296 100.00 11.056
#13857 3.746 0.863 56.74 0.10 3.270 4.040 3.403 43.23 10.707
#14505 3.564 0.014 100.00 0.80 2.920 10.060 7.757 100.00 10.025
#14668 4.600 0.209 99.56 0.10 1.870 5.230 4.789 99.53 10.177
#14722 4.145 1.816 5.23 0.40 4.110 4.180 0.617 0.36 10.180
#14793 4.474 1.225 27.41 0.00 4.040 5.160 9.185 0.01 11.411
#15541 3.949 1.216 27.45 0.40 3.690 4.110 0.680 0.00 11.146
#15761 4.292 0.177 99.78 0.10 3.900 4.530 6.567 0.00 11.126
#15771 3.564 0.360 96.35 0.20 3.060 3.830 6.854 0.00 11.283
See Table 3 for the column description. For the objects with extremely high redshift best fit solutions, the same caveat we gave in Table 3 should be taken into account.
a These values for the galaxy masses were found for the secondary solutions of photometric redshift, because the hyperzmass software did not find a acceptable solution at $z\sim 9{-}10$.

Source LaTeX | All tables | In the text

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