Table 2
Derived properties of EELGs in zCOSMOS.
| zCOSMOS ID | MT | M B | log LFUV | r 50 | log M∗ | log SFRHα,Hβ | c(Hβ) | 12 + log(O/H) | Method |
| mag | L ⊙ | kpc | M ⊙ | M⊙ yr-1 | |||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
|
|
|||||||||
| 700882 | T | –18.9 | 10.23 | 1.02 | 8.66±0.12 | 0.45± 0.18 | 0.28±0.18b | ... | ... |
| 701051 | T | –18.06 | 9.88 | 1.48 | 8.32±0.11 | 0.38± 0.03 | 0.59±0.04a | ... | ... |
| 701741 | ... | –18.94 | 10.15 | ... | 8.41±0.05 | 0.8± 0.11 | 0.12±0.11b | 7.46±0.15 | T e |
| 800984 | T | –19.04 | 10.5 | 1.54 | 8.76±0.01 | 1.03± 0.07 | 0.36±0.07c | 7.95±0.07 | T e |
| 801094 | ... | –19.27 | 10.29 | ... | 8.77±0.17 | –0.14±0.13 | 0.17±0.13b | 8.14±0.1 | R23 |
| 802275 | M | –19.93 | 10.7 | 2.22 | 9.14±0.06 | 1.13± 0.08 | 0.54±0.08c | 8.18±0.06 | R23 |
| 803226 | C | –19.5 | 10.13 | 1.72 | 8.86±0.19 | 0.41± 0.07 | 0.20±0.07b | 7.87±0.1 | T e |
| 803892 | C | –18.96 | 9.96 | 1.43 | 8.55±0.23 | 0.19± 0.09 | 0.24±0.09b | ... | ... |
| 804130 | M | –20.08 | 9.98 | 2.21 | 9.01±0.07 | 0.33± 0.16 | 0.45±0.09c | 8.53±0.12 | N2 |
| 804791 | C | –20.65 | 11.05 | 2.02 | 9.47±0.05 | 0.51± 0.06 | 0.05±0.06b | 8.29±0.16 | R23 |
Notes. Columns: (1) zCOSMOS identification number; (2) morphological type: (R) Round/Nucleated, (C) Clumpy/Chain, (T) Cometary/Tadpole, (M) Merger/Interacting;(3) rest-frame absolute B-band magnitude. Median 1σ uncertainties are ~0.07 mag; (4) rest-frame, dust-corrected FUV luminosity. Median 1σ uncertainties are ~0.11 dex; (5) circularized effective radius. Median 1σ uncertainties are ~10%; (6) stellar mass from SED fitting (Chabrier 2003 IMF); (7) star formation rate from Hα or Hβ luminosity (Chabrier 2003 IMF); (8) reddening constant derived from or (a) and (b) cannot be measured or where they produce a negative extinction (i.e., Hα/Hβ< 2.82 or Hγ/Hβ< 0.47, assuming Case B recombination with Te = 2 × 104 K, ne = 100 cm-3); (9) gas-phase metallicity. The uncertainties quoted for 12+log(O/H) only take into account the propagation of errors from the emission line flux measurements; (10) method used for metallicity derivation (see text for details). The entire version of this table for the full sample of EELGs is available at the CDS.
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