Table 5.
Lens masses ML and distances DL for best fitting models for Gaia18cbf.
| Parameter | GF+ | GF− |
|---|---|---|
| Gblend [mag] |
 |
 |
| Mass function ∝M−1.75, 14.5 kpc < DS < 23.0 kpc | ||
| ML [M⊙] |
 |
 |
| DL [kpc] |
 |
 |
| Gblend, MS [mag] | 13.94 (B9.5V) | 15.33 (F0V) |
Notes. Here, we assumed the distance to source star found in Sect. 4. Gblend is the limit for the brightness of the lens and Gblend, MS is brightness of the lens if it was a MS star of mass similar to ML located at the median distance DL. We assumed that extinction changes with the distance (see Sect. 5). The absolute magnitude in the G-band was taken from PM, and we provide the spectral type of the object used for our calculations in brackets.
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