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Table 2.

Important parameters for the astrometric microlensing events reported here.

Luyten 143-23 (2018) Luyten 143-23 (2021) Ross 322 (2018)
Sou_ID 5254061535052907008 5254061535097574016 314922601464808064
Sou_RA 161.08462829° 161.08436459° 16.95791867°
Sou_Dec −61.20147495° −61.20032468° +34.21100433°
Sou_σRA 0.16 mas 0.06 mas 0.27 mas
Sou_σDec 0.16 mas 0.06 mas 0.38 mas
Sou_µRA −4.85 mas yr −5.20 mas yr −1.12 mas yr
Sou_µDec 2.82 mas yr−1 2.17 mas yr−1 0.83 mas yr−1
Sou_σµRA 0.38 mas yr−1 0.13 mas yr−1 0.60 mas yr−1
σµDec 0.33 mas yr−1 0.12 mas yr−1 0.62 mas yr−1
Sou_ϖ 0.09 mas 0.07 mas −0.05 mas
Sou_σϖ 0.19 mas 0.07 mas 0.44 mas
Sou_G 18.5 mag 17.0 mag 18.6 mag
Sou_GRP 16.9 mag 15.9 mag 17.6 mag
Sou_GBP 19.1 mag 18.0 mag 18.6 mag
θE 14.0 mas 14.0 mas 9.8 mas
σ θE 0.7 mas 0.7 mas 0.5 mas
Tmin (TCB) J2018.51236 yr J2021.18674 yr J2018.5995 yr
σTmin 0.00051 yr 0.00063 yr 0.0022 yr
Dmin 108.5 mas 280.1 mas 125.3 mas
σDmin 1.4 mas 1.1 mas 3.4 mas
Δθmax 1.74 mas 0.69 mas 0.76 mas
σΔθmax 0.12 mas 0.05 mas 0.06 mas

Notes. The table lists source ID (Sou_ID), J2015.5 position (Sou_RA, Sou_Dec), proper motion (Sou_µ) parallax(Sou_ϖ), and G magnitude (Sou_G, Sou_GRP, Sou_GBP) for the background stars. Furthermore, the angular Einstein radii (θE), epoch and distance of closest approach (Tmin, Dmin), and the maximum expected shifts (Δθmax) are shown. Further information for the background stars can be extracted from Gaia DR2 using the Source ID.

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