Table 4
Properties derived from the best-fit SED modelling of our galaxies.
| id_ch2 | z spec | SFR(t) | τ | Age | Av | M ⋆ | PL |
|
| (Gyr) | (yr) | (M⊙ ) | ||||||
|
|
||||||||
| 30555 | 2.640 | e−t/τ | 10.000 | 1.02e+09 | 0.40 | 5.01e+10 | N | 5.45 |
| 34743 | 3.186 | e−t/τ | 0.010 | 1.02e+08 | 0.10 | 2.72e+10 | Y | 5.99 |
| 36718 | 3.209 | e−t/τ | 0.010 | 5.50e+07 | 0.80 | 4.08e+10 | N | 6.94 |
| 37262 | 2.934 | e−t/τ | 0.010 | 7.19e+07 | 0.00 | 9.91e+09 | N | 5.76 |
| 38729 | 2.611 | e−t/τ | 0.100 | 1.43e+08 | 0.60 | 9.19e+09 | N | 2.63 |
| 86032 | 2.696 | e−t/τ | 0.010 | 7.19e+07 | 0.80 | 3.15e+10 | N | 4.54 |
| 92077 | 3.930 | e−t/τ | 0.010 | 1.28e+08 | 0.0. | 1.10e+11 | N | 39.17a |
| 94370 | 2.076 | e−t/τ | 0.010 | 7.19e+07 | 0.80 | 1.02e+10 | N | 4.79 |
| 94971 | 3.100 | e−t/τ | 0.100 | 4.54e+08 | 0.50 | 1.06e+11 | Yb | 4.35 |
| 95692 | 3.284 | e−t/τ | 0.010 | 1.02e+08 | 0.30 | 2.35e+11 | Y | 23.52 |
|
|
||||||||
| 25668 | 3.437 | e−t/τ | 0.010 | 5.50e+07 | 0.00 | 5.15e+09 | N | 5.33 |
| 97267 | 3.090 | e−t/τ | 0.010 | 7.19e+07 | 0.40 | 1.77e+10 | N | 3.06 |
Notes. We used the BC03 models to construct our stellar templates, applied dust reddening according to Calzetti et al. (2000), and used a PL component as explained in Sect. 5. The parameters for the models are given in Table 3. The columns are: (1) the id number of the source; (2) the spectroscopic redshift; (3) the SFH, we consider singles bursts, exponentially declining SFRs and constant SFH; (4) the free parameter for the corresponding SFH; (5) the age; (6) the dust attenuation; (7) the stellar mass; (8) the AGN classification, according to the PL component analysis; (9) the minimum χ2 value.
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