Table A.1.
30 compositions of the lensing galaxy for each of the three source sizes: rs = 0.605 (largest), 0.276 (intermediate), and 0.1 (smallest).
| fsdmG | FpbhG | fstarG | fpbhG | rpbh |
|---|---|---|---|---|
| 0.1 | 0.0 | 0.90 | 0.00 | — |
| 0.1 | 0.81 | 0.09 | −2.5 | |
| −0.5 | ||||
| +1.5 | ||||
| 0.5 | 0.45 | 0.45 | −2.5 | |
| −0.5 | ||||
| +1.5 | ||||
| 0.9 | 0.09 | 0.81 | −2.5 | |
| −0.5 | ||||
| +1.5 | ||||
| 0.5 | 0.0 | 0.50 | 0.00 | — |
| 0.1 | 0.45 | 0.05 | −2.5 | |
| −0.5 | ||||
| +1.5 | ||||
| 0.5 | 0.25 | 0.25 | −2.5 | |
| −0.5 | ||||
| +1.5 | ||||
| 0.9 | 0.05 | 0.45 | −2.5 | |
| −0.5 | ||||
| +1.5 | ||||
| 0.9 | 0.0 | 0.10 | 0.00 | — |
| 0.1 | 0.09 | 0.01 | −2.5 | |
| −0.5 | ||||
| +1.5 | ||||
| 0.5 | 0.05 | 0.05 | −2.5 | |
| −0.5 | ||||
| +1.5 | ||||
| 0.9 | 0.01 | 0.09 | −2.5 | |
| −0.5 | ||||
| +1.5 |
Note: fsdmG, fstarG, and fpbhG are the mass fractions of the galaxy G in SDM, stars, and PBHs, respectively. The stellar mass function follows a Kroupa distribution with a mean mass Mstar = 0.3 M⊙, while all PBHs have the same mass Mpbh, where rpbh = log(Mpbh/Mstar). The relative radius rs is the ratio between the source radius and the Einstein radius (in the source plane) of a typical star with the mean mass Mstar.
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