Table 2
Results from the SED fits for the LBGs.
| LBG_id | Age | A V | log M ⋆ | min  |
SFR | |
| (Myr) | (mag) | (M⊙) | (M⊙ yr-1) | |||
|
|
||||||
| 46190 |
|
|
|
1.09 | 14 ± 0.7 | |
| 47362 |
|
|
|
2.07 | 42 ± 2.0 | |
| 49138 |
|
|
|
8.24 | 5 ± 0.2 | |
| 53929 |
|
|
|
8.89 | 13 ± 0.6 | |
| 58236 |
|
|
|
3.17 | 11 ± 0.5 | |
| 59257 |
|
|
|
0.71 | 39 ± 1.8 | |
| 61554 |
|
|
|
2.69 | 64 ± 3.0 | |
| 61983 |
|
|
|
0.42 | 23 ± 1.1 | |
| 62478 |
|
|
|
2.06 | 25 ± 1.2 | |
| 62522 |
|
|
|
9.21 | 34 ± 1.6 | |
| 63294 |
|
|
|
2.39 | 9 ± 0.4 | |
| 63984 |
|
|
|
1.25 | 12 ± 0.6 | |
| 66235 |
|
|
|
6.61 | 64 ± 6.2 | |
| 69377 |
|
|
|
3.58 | 29 ± 1.4 | |
| 69919 |
|
|
|
1.16 | 42 ± 4.1 | |
Notes. Stellar properties from fitting 2 SSPs to the data. Columns give the age of the younger SSP, dust AV, mass in stars, the minimum reduced χ2 and the dust corrected SFRs as calculated from the UV flux of all the fits. We here only give the age of the younger SSP, as any older stellar population is totally obscured by this younger population. LBGs 49138 and 53929 have been fitted after removing obvious strong emission lines. The bad χ2 of 62522 suffers from odd features in the NIR ISAAC photometry. Both object 53929 and 66235 lie on the edge of the HST imaging field and may thus also have larger systematic uncertainties on the photometry. Please note that the error bars in column six are the pure measurement errors on the U band photometry, and do not incorporate uncertainties in the extrapolation to 1500 Å, or in the SFR conversion factor.
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