Table A.6.
Lens mass and distance estimates of the five candidate dark lens microlensing events, that didn’t pass the πE criterion, but were chosen to be analysed further. Descriptions of the columns are at the end of the table. A machine-readable version of this table is available at the CDS.
GaiaDR3- | MF | ML | DL | GMS | Gblend | θE | δmax | μL | vt | Prob |
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ULENS | [M⊙] | [kpc] | [mag] | [mag] | [mas] | [mas] | [mas yr−1] | [km s−1] | [%] | |
103-G+ | K2001 |
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83.63 |
103-G+ | M2021 |
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97.56 |
103-G+ | ∼M−1 |
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94.48 |
103-G- | K2001 |
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83.12 |
103-G- | M2021 |
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97.52 |
103-G- | ∼M−1 |
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94.43 |
155-G1- | K2001 |
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78.47 |
155-G1- | M2021 |
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97.41 |
155-G1- | ∼M−1 |
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91.21 |
155-G2- | K2001 |
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92.29 |
155-G2- | M2021 |
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98.78 |
155-G2- | ∼M−1 |
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97.54 |
212-GSA+ | K2001 |
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76.06 |
212-GSA+ | M2021 |
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98.07 |
212-GSA+ | ∼M−1 |
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93.12 |
212-GSA- | K2001 |
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84.96 |
212-GSA- | M2021 |
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98.72 |
212-GSA- | ∼M−1 |
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95.84 |
259-GSA+ | K2001 |
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75.25 |
259-GSA+ | M2021 |
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98.59 |
259-GSA+ | ∼M−1 |
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96.37 |
259-GSA- | K2001 |
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66.45 |
259-GSA- | M2021 |
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97.76 |
259-GSA- | ∼M−1 |
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93.48 |
331-G+ | K2001 |
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96.93 |
331-G+ | M2021 |
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99.96 |
331-G+ | ∼M−1 |
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99.85 |
331-G- | K2001 |
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97.38 |
331-G- | M2021 |
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99.97 |
331-G- | ∼M−1 |
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99.89 |
Notes: The columns are event name, mass function MF used as a prior for lens mass, the mass of the lens, ML, in solar masses, distance to the lens, DL, in kpc, the brightness of an MS star with the ML mass at a distance, DL, and the brightness of the blend Gblend obtained from the microlensing model, Einstein radius, θE, maximal astrometric displacement, δmax, proper motion of the lens, μL, transverse velocity, vt, and probability for a dark lens. In the MF column, K2001 refers to Kroupa (2001), and M2021 to Mróz et al. (2021).
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