Table 2.
Lens candidates with X-shooter spectra.
Name | zl | zs | nSérsic | qlight | PAlight | θEin | q | PA |
![]() |
Comment |
---|---|---|---|---|---|---|---|---|---|---|
[deg] | [″] | [deg] | [″] | |||||||
HSCJ022622−042522 | 1.119* | 2.146* | 9.13 | 0.85 | 10.28 | 1.28 | 0.56 | −8.92 | 0.88 | – |
HSCJ023817−054555 | 0.599 | 1.763 | 2.89 | 0.85 | 51.19 | 0.99 | 0.87 | 45.17 | 0.92 | – |
HSCJ091148+041852 | 0.861* | 2.627* | 10.00 | 0.83 | −78.45 | 2.39 | 0.40 | 74.04 | 1.24 | Found by YATTALENS |
HSCJ115252+004733 | 0.466 | 3.760 | 3.63 | 1.00 | −86.82 | 3.28 | 0.33 | 19.22 | 1.45 | More et al. (2017) |
HSCJ141136−010216 | 0.949* | 3.021* | 6.48 | 0.56 | −52.30 | 1.28 | 0.74 | −47.67 | 1.07 | Found by YATTALENS |
HSCJ144320−012538 | 0.890* | 1.703* | 2.76 | 0.73 | −52.94 | 1.68 | 0.52 | −56.09 | 1.09 | – |
Notes. We measure the lens and source redshifts as shown in Cols. 2 and 3. We highlight the new redshift measurements with an asterisk. The best-fit parameter values of lens modeling from GLEE are listed in Cols. 4−9, as illustrated in Fig. 4. The corresponding scaled Einstein radius as listed in Col. 10. We allow for an additional external shear component for HSCJ022622−042522 and find γext = 0.15 and PAext = 52.27deg, due to the presence of a close-by galaxy group.
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