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Table 3
Fits with the assumption of the Lorentzian and Gaussian shape for Hβ broad component.
| Name | Stellar | Starlight | EW(FE) | EW(Hβ) | RFe | FWHM | χ2 | Starlight | EW(FE) | EW(Hβ) | RFe | FWHM | χ2 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| age [Gyr] | [%] | [km s−1] | d.o.f. | [%] | [km s−1] | d.o.f. | |||||||
| 0147 | 0.005 | 7.5 | 34.8 | 37.5 | 0.9 | 2034 | 4.99 | 7.7 | 33.1 | 27.1 | 1.2 | 2664 | 5.12 |
| 0200 | 13.000 | 1.2 | 44.4 | 40.9 | 1.1 | 1566 | 3.56 | 1.3 | 41.8 | 30.3 | 1.4 | 2345 | 3.75 |
| 0354 | 0.001 | 5.8 | 46.3 | 76.4 | 0.6 | 2266 | 1.98 | 5.5 | 38.1 | 54.0 | 0.7 | 2684 | 1.94 |
| 0849 | 0.025 | 11.4 | 43.9 | 50.6 | 0.9 | 2128 | 1.53 | 1.3 | 41.5 | 37.3 | 1.1 | 2743 | 1.61 |
| 1005 | 0.010 | 30.0 | 73.6 | 63.2 | 1.2 | 1930 | 3.06 | 29.9 | 63.6 | 48.8 | 1.3 | 2732 | 3.79 |
| 1030 | 0.003 | 15.1 | 53.2 | 79.6 | 0.7 | 2902 | 1.63 | 15.1 | 44.9 | 60.6 | 0.7 | 3690 | 1.83 |
| 1050 | 0.001 | 44.2 | 133.9 | 177.8 | 0.8 | 2708 | 4.77 | 44.8 | 142.6 | 147.0 | 1.0 | 3233 | 4.37 |
| 1052 | 0.001 | 50.3 | 146.1 | 110.1 | 1.3 | 5392 | 5.11 | 51.1 | 136.0 | 87.2 | 1.6 | 5020 | 4.44 |
| 1100 | 0.001 | 21.6 | 42.9 | 28.4 | 1.5 | 1502 | 1.55 | 21.6 | 34.3 | 18.3 | 1.9 | 1620 | 1.48 |
| 1111 | 0.001 | 69.1 | 220.0 | 187.6 | 1.2 | 3828 | 3.43 | 64.7 | 220.2 | 171.5 | 1.3 | 4502 | 2.83 |
| 1207 | 0.102 | 10.9 | 43.1 | 33.9 | 1.3 | 1398 | 2.34 | 15.3 | 50.1 | 26.8 | 1.9 | 2099 | 2.30 |
| 1209 | 0.001 | 47.4 | 77.2 | 87.7 | 0.9 | 4212 | 2.36 | 43 | 72.0 | 68.2 | 1.1 | 5065 | 2.07 |
| 1215 | 11.000 | 11.7 | 24.2 | 28.7 | 0.8 | 1030 | 3.99 | 15 | 26.7 | 22.0 | 1.2 | 1555 | 4.39 |
| 1251 | 0.010 | 56.6 | 91.37 | 124.70 | 0.7 | 1377 | 4.38 | 54.3 | 46.44 | 79.75 | 0.6 | 2025 | 8.71 |
| 1253* | 0.001 | 47.4 | 12.2 | 315.1 | 0.0 | 9118 | 3.66 | 50.7 | 10.5 | 210.8 | 0.0 | 8863 | 4.26 |
| 1301 | 0.025 | 65.6 | 190.0 | 196.2 | 1.0 | 2318 | 5.54 | 62.8 | 170.0 | 157.9 | 1.1 | 3517 | 6.45 |
| 1314 | 2.500 | 9.8 | 40.6 | 51.3 | 0.8 | 3124 | 2.09 | 9.8 | 36.5 | 39.2 | 0.9 | 3584 | 1.86 |
| 1330 | 0.001 | 92.4 | 975.2 | 1199.4 | 0.8 | 9404 | 1.43 | 88.5 | 530.2 | 565.9 | 0.9 | 9742 | 1.24 |
| 1347 | 0.102 | 36.1 | 48.7 | 45.8 | 1.1 | 1640 | 8.32 | 36.3 | 43.7 | 34.8 | 1.3 | 2048 | 8.60 |
| 1417 | 0.010 | 35.9 | 83.5 | 132.2 | 0.6 | 3106 | 3.80 | 50.7 | 126.5 | 133.2 | 0.9 | 3537 | 3.41 |
| 1419 | 0.286 | 69.5 | 117.0 | 370.4 | 0.3 | 4258 | 2.60 | 67.8 | 91.2 | 280.9 | 0.3 | 4885 | 2.36 |
| 1446 | 0.010 | 78.2 | 307.9 | 374.5 | 0.8 | 2412 | 6.03 | 74.4 | 208.0 | 197.1 | 1.1 | 3968 | 5.89 |
| 1502 | 0.010 | 20.5 | 44.5 | 21.0 | 2.1 | 936 | 1.09 | 26.7 | 51.0 | 17.2 | 3.0 | 1445 | 1.02 |
| 1515 | 0.001 | 26.6 | 56.2 | 107.6 | 0.5 | 2816 | 1.38 | 26.6 | 49.9 | 78.3 | 0.6 | 2945 | 1.32 |
| 1529 | 0.001 | 20.8 | 34.5 | 72.3 | 0.5 | 5076 | 1.25 | 21.5 | 45.6 | 86.2 | 0.5 | 6603 | 1.16 |
| 1652 | 0.025 | 41.2 | 280.4 | 271.5 | 1.0 | 9292 | 4.61 | 37.3 | 220.1 | 142.3 | 1.3 | 8457 | 4.36 |
| 2130 | 0.010 | 54.8 | 66.6 | 107.9 | 0.6 | 3104 | 2.02 | 54.6 | 58.0 | 82.0 | 0.7 | 3746 | 1.44 |
Notes. (*) The results for this object reported in the Shen et al. (2011) catalog were incorrect due to a software problem (Yue Shen, private communication).
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