Table 5
Fitting results for the classic scenario model, meaning using Calzetti, constant star formation, no nebular emission, and tmin = 100 Myr, obtained as in Table 4.
ID |
![]() |
A V | Age [Gyr] | M⋆ [1010 M⊙] | Lbol[1011 L⊙] | SFRBC[M⊙ yr-1] | SFRIR[M⊙ yr-1] |
|
|||||||
A68/C0 | 1.09 | 1.6 (1.4−1.8) | 0.51 (0.255−1.01) | 2.76 (2.04−3.57) | 3.74 (2.59−5.53) | 62.8(42−97.1) | 20.4 (19.2−21.5) |
A68/h7 | 3.33 | 1.9 (1.8−2.0) | 0.18 (0.13−0.25) | 20.3 (17.7−24.3) | 71.3 (57.9−85.7) | 1308 (1035−1623) | 315 (294−330) |
A68/HLS115 | 1.92 | 1.8 (1.7−1.9) | 0.18 (0.13−0.36) | 1.7 (1.4−2.1) | 5.42 (4.2−6.7) | 96.3(73−128.3) | 59.0 (56.3−61.7) |
A68/nn4 | 6.16 | 2.4 (2.3−2.4) | 0.25 (0.25−0.36) | 20.3 (18.6−24.9) | 51.1 (44.5−56.0) | 878.7 (729.6−962.6) | 1184 (1132−1214) |
MACS0451 | 40.7 | 0.7 (0.6−0.7) | 0.18 (0.18−0.36) | 0.52 (0.51−0.75) | 1.38 (1.04−1.41) | 33.2(25.2−33.6) | 15−42 |
cB58 | 3.92 | 0.6 (0.6−0.7) | 0.25 (0.18−0.25) | 1.07 (0.88−1.14) | 2.1 (1.96−2.7) | 52.3(48.8−64) | 52.4 (51.2−53.6) |
Cosmic Eye | 1.94 | 0.8 (0.8−0.8) | 0.36 (0.36−0.36) | 4.14 (4.0−4.25) | 6.65 (6.5−6.8) | 139.4 (136.1−143.1) | 58.8 (54.9−61.6) |
Notes. Values are corrected for lensing. The SFRIR from Table 3 is also listed for comparison. The results listed for MACS0451 come from the integrated photometry of the entire arc, and that a scaling factor 0.4 can be applied to estimate the properties of the northern part separately (see Sect. 5.1.5). For MACS0451, SFRIR corresponds to the range given by the LIR of the northern segment and that of the whole arc.
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