Table 4:
Additional best fits of RV and E(B-V) together with the
1
uncertainties for quasar images which are likely to be dust
extincted. The first three quasar images are badly described when
using both HST and ground-based images, but are possible to fit with
dust when using only the ground-based measurements. The last image is
one where the u band magnitude seems to be deviant from the other
magnitudes and we have made a fit without it.
| Quasar |
Image |
 |
d (kpc) |
RV |
E(B-V) |
Law |
Prob |
Comment |
| HE0230-2130 |
A2 |
0.52 |
6.1 |
3.2 (1.5-5.4) |
0.2 (0.1-0.2) |
CCM |
13% |
ground |
| HE0230-2130 |
A2 |
0.52 |
6.1 |
3.4 (1.8-6.0) |
0.2 (0.1-0.2) |
Fitzpatrick |
12% |
ground |
| HE0230-2130 |
A2 |
0.52 |
6.1 |
4.0 (1.6-6.0) |
0.2 (0.1-0.3) |
SMC |
15% |
ground |
| HE0230-2130 |
A2 |
2.16 |
6.1 |
0.1 (0.1-3.0) |
0.1 (0.1-0.1) |
Host CCM |
1% |
ground |
| HE0230-2130 |
A2 |
2.16 |
6.1 |
1.7 (0.4-2.8) |
0.1 (0.0-0.1) |
Host Fitzpatrick |
4% |
ground |
| HE0230-2130 |
A2 |
2.16 |
6.1 |
6.0 (0.1-6.0) |
0.1 (0.1-0.1) |
Host SMC |
4% |
ground |
| HE0230-2130 |
B |
0.52 |
8.0 |
2.6 (0.5-4.2) |
0.3 (0.2-0.3) |
CCM |
1% |
ground |
| HE0230-2130 |
B |
0.52 |
8.0 |
2.9 (0.7-5.7) |
0.3 (0.1-0.3) |
Fitzpatrick |
1% |
ground |
| HE0230-2130 |
B |
0.52 |
8.0 |
3.7 (1.4-6.0) |
0.3 (0.2-0.3) |
SMC |
1% |
ground |
| HE0230-2130 |
B |
2.16 |
8.0 |
6.0 (0.1-6.0) |
0.1 (0.1-0.1) |
Host SMC |
1% |
ground |
| SDSS J144612.98+035154.4 |
A |
1.51 |
- |
2.0 (0.1-2.0) |
0.2 (0.1-0.3) |
CCM |
26% |
no u |
| SDSS J144612.98+035154.4 |
A |
1.51 |
- |
2.0 (1.4-2.0) |
0.2 (0.1-0.2) |
Fitzpatrick |
32% |
no u |
| SDSS J144612.98+035154.4 |
A |
1.95 |
- |
1.1 (0.9-1.5) |
0.1 (0.1-0.1) |
Host Fitzpatrick |
9% |
no u |
Source LaTeX |
All tables |
In the text