Table 1:
The basic properties of the 27 combined spectra.
Columns (1)-(6) refer to the counting number,
the label for the mass bin (marked in Fig. 1),
the mass bin, the average
EW([O II]
3727) of the sample galaxies in each
bin, the total number of the galaxies, and
the number of the selected spectra to be combined (about half) in each bin,
respectively.
(1) |
(2) |
(3) |
(4) |
(5) |
(6) |
No. |
Label |
Mass bin |
EW([O II]) |
Total |
Selected |
|
|
(log M*) |
average (Å) |
number |
number |
1 |
m87 |
<8.7 |
-78.72 |
378 |
149 |
2 |
m871 |
8.7-8.8 |
-73.73 |
339 |
158 |
3 |
m881 |
8.8-8.9 |
-71.53 |
533 |
228 |
4 |
m891 |
8.9-9.0 |
-65.51 |
797 |
341 |
5 |
m901 |
9.0-9.1 |
-62.24 |
1227 |
533 |
6 |
m911 |
9.1-9.2 |
-60.42 |
1470 |
593 |
7 |
m921 |
9.2-9.3 |
-57.76 |
1885 |
766 |
8 |
m931 |
9.3-9.4 |
-55.02 |
2428 |
1029 |
9 |
m9405 |
9.40-9.45 |
-52.80 |
1329 |
552 |
10 |
m94505 |
9.45-9.50 |
-51.31 |
1478 |
627 |
11 |
m9505 |
9.50-9.55 |
-50.41 |
1670 |
705 |
12 |
m95505 |
9.55-9.60 |
-48.14 |
1746 |
751 |
13 |
m9605 |
9.60-9.65 |
-46.58 |
1920 |
814 |
14 |
m96505 |
9.65-9.70 |
-45.11 |
2001 |
837 |
15 |
m9705 |
9.70-9.75 |
-43.72 |
2156 |
906 |
16 |
m97505 |
9.75-9.80 |
-42.17 |
2262 |
951 |
17 |
m9805 |
9.80-9.85 |
-40.21 |
2428 |
1010 |
18 |
m98505 |
9.85-9.90 |
-38.31 |
2841 |
1020 |
19 |
m9905 |
9.90-9.95 |
-35.94 |
2552 |
1025 |
20 |
m99505 |
9.95-10.0 |
-33.59 |
2605 |
1048 |
21 |
m10005 |
10.0-10.05 |
-33.22 |
2750 |
1076 |
22 |
m100505 |
10.05-10.10 |
-31.19 |
2814 |
1120 |
23 |
m1011 |
10.10-10.20 |
-29.12a |
5860 |
2145 |
24 |
m1021 |
10.20-10.30 |
-26.28a |
6004 |
1813 |
25 |
m1031 |
10.30-10.40 |
-23.79a |
6084 |
1417 |
26 |
m1041 |
10.40-10.50 |
-22.18a |
5973 |
1148 |
27 |
m1051 |
10.50-10.60 |
-20.72a |
5341 |
846 |
a For the massive galaxies with log(M*)>10.10,
we select those with
stronger [O II] emission-lines with EW([O II])< -30 Å for spectral combination.
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