Stellar massa | SFR(![]() |
Rest frame B | |||||||||
Our ID | z |
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(
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HRb | B/T |
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Typec | Qd |
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M1/M2f |
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) |
904260 | 0.983 | 10.32 | <10.37 | 3.62 < ![]() |
- | - | S | 3 | M2 | ||
904604 | 0.990 | 10.94 | <10.59 | 0.13 < ![]() |
0.33 ![]() |
1.063 | S | 1 | 2.53 ![]() |
||
904680 | 0.964 | 10.28 | <9.83 | 3.28 < ![]() |
- | - | 4 | M2 | |||
905632 | 0.976 | 10.23 | <10.18 | 0.87 < ![]() |
0.33 ![]() |
1.093 | S | 1 | 1.16 ![]() |
||
905983 | 0.860 | 10.36 | <7.22 | 3.87 < ![]() |
0.08 ![]() |
1.129 | S | 2 | 1.85 ![]() |
||
906961g | 0.566 | 10.81 | 70.36 | < 120 | -0.55 ![]() |
- | - | E | - | ||
907047 | 1.112 | 10.65 | <14.49 | 3.32 < ![]() |
- | - | 4 | M1 | |||
907361 | 0.731 | 10.96 | <6.69 | 0.18 < ![]() |
0.80 ![]() |
1.322 | E | 2 | |||
907794 | 1.144 | 10.92 | 20.82 | 35 | 0.67 ![]() |
1.099 | S0 | 1 | |||
908243 | 0.726 | 10.23 | <6.57 | 2.41 < ![]() |
0.13 ![]() |
1.195 | Tad | 3 | |||
909015 | 1.039 | 10.25 | <12.07 | 0.29 < ![]() |
- | - | 4 | ||||
909093 | 0.968 | 9.71 | <9.97 | 3.37 < ![]() |
0.65 ![]() |
1.093 | Tad | 3 | |||
909429 | 0.737 | 10.32 | <6.81 | 4.48 < ![]() |
- | - | 4 | M2 | |||
910413 | 0.655 | 10.67 | 15.84 | 27 | - | - | Tad | 4 | M2 | ||
911747 | 0.840 | 10.18 | <6.79 | 4.81 < ![]() |
- | - | 4 | M2 | |||
911780 | 0.664 | 10.38 | <5.29 | 3.69 < ![]() |
0.26 ![]() |
1.295 | S | 2 | 2.34 ![]() |
||
911843 | 0.973 | 9.75 | <10.09 | 5.50 < ![]() |
- | - | 4 | M2 | |||
912744 | 0.690 | 10.40 | <5.81 | 2.31 < ![]() |
- | - | S | 3 | |||
913482 | 0.664 | 10.71 | 27.17 | < 46 | 0.52 ![]() |
0.48 ![]() |
1.221 | S0 | 3 | ||
914038 | 0.667 | 10.50 | 12.00 | 20 | - | - | 4 | M2 | |||
915400 | 0.764 | 10.42 | <7.44 | 1.73 < ![]() |
0.08 ![]() |
1.333 | S | 2 | 2.45 ![]() |
||
916137 | 0.980 | 10.33 | <10.29 | 1.40 < ![]() |
0.60 ![]() |
1.094 | Irr | 3 | |||
916446 | 0.839 | 10.10 | <6.77 | 1.75 < ![]() |
- | - | 4 | M2 | |||
916866 | 0.987 | 10.22 | <10.48 | 1.68 < ![]() |
0.42 ![]() |
1.137 | S0 | 2 | |||
918147 | 1.099 | 10.77 | 39.48 | 67 | - | - | 4 | M1 | |||
919573 | 0.665 | 10.61 | 5.89 | < 10 | -0.40 ![]() |
0.61 ![]() |
1.172 | S0 | 3 | ||
919595 | 0.785 | 10.24 | <7.95 | 2.43 < ![]() |
0.12 ![]() |
1.182 | S | 3 | |||
920435 | 1.034 | 9.44 | <11.91 | 2.66 < ![]() |
0.49 ![]() |
1.116 | S0 | 2 | |||
921406 | 1.095 | 10.37 | <13.89 | 5.22 < ![]() |
0.31 ![]() |
1.125 | S | 1 | 2.43 ![]() |
||
922675 | 0.666 | 10.13 | <5.32 | 2.79 < ![]() |
0.47 ![]() |
1.142 | S0 | 1 | |||
922733 | 0.650 | 10.05 | <5.01 | 2.24 < ![]() |
- | - | 4 | M2 | |||
922761 | 0.961 | 9.71 | <9.77 | 2.56 < ![]() |
0.24 ![]() |
1.095 | Irr | 3 | |||
923085 | 1.122 | 10.68 | 15.74 | 26 | 0.87 ![]() |
1.212 | Irr | 3 | |||
923926 | 1.012 | 10.74 | <11.23 | 1.17 < ![]() |
0.12 ![]() |
0.64 ![]() |
1.113 | S0 | 3 | ||
924881 | 0.839 | 9.80 | <6.77 | 2.95 < ![]() |
0.78 ![]() |
1.277 | E | 2 | |||
926109 | 0.522 | 10.19 | <2.95 | 1.55 < ![]() |
- | - | 4 | M1 | |||
926217 | 0.767 | 10.27 | <7.50 | 1.84 < ![]() |
0.50 ![]() |
1.119 | S0 | 1 | |||
907305 | 1.185 | 10.11 | <17.21 | 3.17 < ![]() |
- | - | 4 | M1 | |||
914895 | 0.736 | 10.09 | <6.78 | 2.36 < ![]() |
- | - | 4 | M1 |
a Derived using a diet Salpeter IMF. In order to derive values using a classic Salpeter IMF, add 0.15 dex to the values listed here. b X-ray hardness ratio, defined as (H-S)/(H+S) where H and S are the counts in the hard and soft bands respectively. c Galaxy type - E: 0.8 ![]() ![]() ![]() d Q quality factor - 1: secure; 2: possibly secure; 3: insecure; 4: fit failed. e Exponential disk scale length(kpc) for disk dominated galaxies. f Merging? - M1: obvious merging; M2: possible merging. g This object could not be fitted properly due to the presence of a strong point source at the center. |