Table 5.
Mass measurements on the strong lenses in our sample.
Name | log ![]() |
REin | log MEin | log ![]() |
---|---|---|---|---|
log M⊙ | (kpc) | log M⊙ | log M⊙ | |
015618−010747 | 11.72 ± 0.07 | 5.36 | 11.40 | 11.13 ± 0.07 |
020241−064611 | 11.31 ± 0.11 | 7.09 | 11.48 | 11.14 ± 0.11 |
021411−040502 | 11.66 ± 0.06 | 8.40 | 11.68 | 11.16 ± 0.06 |
021737−051329 | 11.56 ± 0.10 | 8.67 | 11.72 | 11.26 ± 0.10 |
022346−053418 | 11.67 ± 0.10 | 8.96 | 11.78 | 11.29 ± 0.10 |
022610−042011 | 11.62 ± 0.09 | 6.30 | 11.51 | 11.22 ± 0.09 |
023307−043838 | 11.65 ± 0.09 | 12.07 | 12.01 | 11.37 ± 0.09 |
023817−054555 | 11.59 ± 0.10 | 6.21 | 11.43 | 11.35 ± 0.10 |
085855−010208 | 11.39 ± 0.08 | 5.92 | 11.42 | 11.10 ± 0.08 |
094427−014742 | 11.32 ± 0.10 | 4.60 | 11.26 | 10.93 ± 0.10 |
120623+001507 | 11.70 ± 0.11 | 7.55 | 11.52 | 11.20 ± 0.11 |
121052−011905 | 11.70 ± 0.11 | 9.14 | 11.73 | 11.29 ± 0.11 |
121504+004726 | 11.60 ± 0.07 | 10.48 | 11.99 | 11.44 ± 0.07 |
140929−011410 | 11.41 ± 0.11 | 8.19 | 11.62 | 11.11 ± 0.11 |
141300−012608 | 11.61 ± 0.11 | 8.32 | 11.63 | 11.24 ± 0.11 |
141815+015832 | 11.44 ± 0.10 | 8.99 | 11.71 | 11.22 ± 0.10 |
142449−005321 | 12.07 ± 0.08 | 16.06 | 12.46 | 11.73 ± 0.08 |
142720+001916 | 11.55 ± 0.07 | 8.98 | 11.83 | 11.35 ± 0.07 |
144307−004056 | 11.44 ± 0.08 | 6.69 | 11.61 | 11.22 ± 0.08 |
220506+014703 | 11.26 ± 0.09 | 10.07 | 11.80 | 11.14 ± 0.09 |
222801+012805 | 11.61 ± 0.10 | 11.97 | 11.95 | 11.41 ± 0.10 |
223733+005015 | 11.73 ± 0.10 | 8.65 | 11.68 | 11.28 ± 0.10 |
230335+003703 | 11.51 ± 0.10 | 5.98 | 11.55 | 11.10 ± 0.10 |
Notes. From left to right these are stellar mass inferred from stellar population synthesis fitting of HSC photometry, Einstein radius in physical units, total projected mass enclosed within the Einstein radius, and stellar population synthesis stellar mass enclosed within an aperture equal to the Einstein radius.
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