Table 1.
Models used during the photometric redshift estimation with template fitting.
| Model | Description | Filename |
|---|---|---|
| 1 | Elliptical | Ell1_A_0 |
| 2 | ” | Ell2_A_0 |
| 3 | ” | Ell3_A_0 |
| 4 | ” | Ell4_A_0 |
| 5 | ” | Ell5_A_0 |
| 6 | ” | Ell6_A_0 |
| 7 | ” | Ell7_A_0 |
| 8 | Disk | S0_A_0 |
| 9 | Spiral | Sa_A_0 |
| 10 | ” | Sa_A_1 |
| 11 | ” | Sb_A_0 |
| 12 | ” | Sb_A_1 |
| 13 | ” | Sc_A_0 |
| 14 | ” | Sc_A_1 |
| 15 | ” | Sc_A_2 |
| 16 | ” | Sd_A_0 |
| 17 | ” | Sd_A_1 |
| 18 | ” | Sd_A_2 |
| 19 | Irregular | Sdm_A_0 |
| 20 | Extreme starforming | SB0_A_0 |
| 21 | ” | SB1_A_0 |
| 22 | ” | SB2_A_0 |
| 23 | ” | SB3_A_0 |
| 24 | ” | SB4_A_0 |
| 25 | ” | SB5_A_0 |
| 26 | ” | SB6_A_0 |
| 27 | ” | SB7_A_0 |
| 28 | ” | SB8_A_0 |
| 29 | ” | SB9_A_0 |
| 30 | ” | SB10_A_0 |
| 31 | ” | SB11_A_0 |
| 32 | Spiral | CB1 |
| 33 | Disk | S0 |
| 34 | Spiral | Sb |
| 35 | Spiral | Spi4 |
| 36 | AGN | M82 |
| 37 | Starburst/AGN | I22491 |
| 38 | Seyfert 1.8 | Sey18 |
| 39 | Seyfert 2.0 | Sey2 |
| 40 | Disk-obscured QSO Hybrid | S0_90_QSO2_10 |
| 41 | ” | S0_80_QSO2_20 |
| 42 | ” | S0_70_QSO2_30 |
| 43 | ” | S0_60_QSO2_40 |
| 44 | ” | S0_50_QSO2_50 |
| 45 | ” | S0_40_QSO2_60 |
| 46 | ” | S0_30_QSO2_70 |
| 47 | ” | S0_20_QSO2_80 |
| 48 | ” | S0_10_QSO2_90 |
| 49 | AGN | Mrk231 |
| 50 | Starforming-unobsc. QSO Hybrid | I22491_90_TQSO1_10 |
| 51 | ” | I22491_80_TQSO1_20 |
| 52 | ” | I22491_70_TQSO1_30 |
| 53 | ” | I22491_60_TQSO1_40 |
| 54 | ” | I22491_50_TQSO1_50 |
| 55 | ” | I22491_40_TQSO1_60 |
| 56 | ” | pl_I22491_30_TQSO1_70 |
| 57 | ” | pl_I22491_20_TQSO1_80 |
| 58 | ” | pl_I22491_10_TQSO1_90 |
| 59 | QSO | pl_QSOH |
| 60 | QSO | pl_QSO |
| 61 | QSO | pl_TQSO1 |
Notes. Left hand side: normal galaxy models. The starformation increases from top to bottom (see Ilbert et al. 2009 for more details). Right hand side: normal, AGN-QSO and hybrid models. The AGN fraction varies from 0–100% as noted in the name of the model, e.g. S0_90_QSO2_10 is a combination of 90% flux from a disk galaxy and 10% flux contribution from an obscured QSO. The prefix “pl_” denotes that the model has been extended to the ultra-violet assuming a power-law (see Salvato et al. 2009 for a detailed description).
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