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Table A.1.

List of 30 especially promising astrometric microlensing events.

# Source ID Sou_source ID ST M θE σθE T − 2000 σT dmin σdmin δθc,  lum σδθc,  lum δθ+ σδθ+ Δm σΔm
M mas mas Jyear Jyear mas mas mas mas mas mas mag mag
1 478978296199510912 478978296204261248 WD 0.65 15.5 1.8 14.6923 0.0024 50.7 1.1 1.78 0.27 4.34 0.67 0.0055 0.0023
2 4733794485572154752 4733794485572154624 BD 0.07 8.9 1.9 16.0744 0.0099 21.1 7.7 1.68 0.61 3.2 1.3 0.021 0.027
3 5862333044226605056 5862333048529855360 MS 0:400 4:66 0:24 19:417 0:012 6:4 3:5 0:184 0:069 2:44 0:76 0:011 0:015
4 5840411363658156032 5840411359350016128 MS 0.174 3.56 0.18 19.8392 0.0029 5.8 1.3 0.505 0.079 1.69 0.27 0.032 0.020
5 4687445500635789184 4687445599404851456 WD 0.65 13.6 1.7 21.5001 0.0062 70.3 1.9 0.98 0.16 2.52 0.41 0.00101 0.00044
6 4248799013208327424 4248799013215266176 MS 0.219 4.10 0.23 29.876 0.039 0.9 10.0 0.9 3.8 3.7 4.4 0.9 7.8
7 5918299904067162240 5918299908365843840 MS 0.113 6.93 0.35 30.2480 0.0032 6.3 2.8 2.17 0.17 4.46 0.84 0.28 0.22
8 6130500670360253312 6130500567281038080 MS 0.318 2.16 0.33 35.162 0.072 0.2 7.4 0.4 4.3 2.0 3.5 1.0 24.0
9 5863711561290571008 5863711561290570112 MS 0.199 3.39 0.17 35.333 0.014 5.0 3.4 1.179 0.087 1.70 0.69 0.13 0.22
10 4472832130942575872 4472836292758713216 MS 0.184 28.7 1.5 35.76441 0.00073 335.0 13.0 0.0802 0.0065 2.43 0.20 3.69E-6 9.3E-7
11 6074397471079635328 6074397471080379776 WD 0.65 8.3 1.1 36.72 0.26 9.5 40.0 1.7 2.6 5.0 10.0 0.10 0.87
12 5556349476589422336 5556349472293892224 WD 0.65 7.94 0.96 37.173 0.077 15.0 47.0 2.1 3.2 3.7 8.2 0.06 0.57
13 5886942661427781760 5886942661374132096 MS 0.180 3.69 0.19 39.266 0.049 0.2 13.0 0.5 8.0 3.5 5.9 1.0 35.0
14 5715906236031073280 5715906236031079040 WD 0.65 7.85 0.91 40.049 0.034 20.0 6.9 2.06 0.51 2.71 0.84 0.026 0.030
15 5332606522595645952 5332606277747043456 WD 0.65 33.7 3.9 40.7896 0.0021 139.6 4.9 0.0470 0.0077 7.7 1.3 3.4E-5 1.6E-5
16 4118914220102650624 4118914185707335040 MS 0.319 7.11 0.36 41.383 0.014 0.1 13.0 0.07 5.1 7.1 6.5 0.8 92.0
17 428051391503714432 428051391509474816 WD 0.65 8.18 0.97 43.61 0.11 47.0 29.0 1.27 0.71 1.39 0.83 0.0017 0.0040
18 5605383430285597696 5605383537671689856 WD 0.65 15.0 1.7 43.9735 0.0091 207.6 4.5 1.04 0.17 1.08 0.18 5.6E-5 2.7E-5
19 6282457918962299776 6282457815883084928 WD 0.65 19.9 2.3 45.466 0.012 22.0 10.0 1.53 0.43 11.7 3.0 0.032 0.033
20 3365063724883180288 3365062964671171712 MS 0.119 11.08 0.56 45.607 0.011 119.0 14.0 0.0095 0.0013 1.02 0.14 1.46E-6 7.1E-7
21 1822711900548572544 1822711900548570624 MS 0.212 2.37 0.15 49.80 0.27 0.3 44.0 0.3 17.0 2.0 20.0 0.8 100.0
22 4203875751318123904 4203875648238893696 BD 0.07 5.1 1.1 53.538 0.018 11.0 22.0 1.2 1.5 2.1 3.1 0.04 0.22
23 4117081643422165120 4117081467277401344 WD 0.65 11.7 1.4 56.982 0.027 66.0 25.0 1.45 0.54 1.99 0.77 0.0014 0.0021
24 6126095232211644160 6126095300931121024 WD 0.65 5.68 0.73 57.33 0.27 4.6 32.0 1.52 0.22 3.8 9.8 0.2 2.9
25 6426625402561169024 6426625402559392896 MS 0.272 4.94 0.25 58.252 0.017 4.5 4.2 1.12 0.20 3.2 1.3 0.16 0.28
26 5243594081269535872 5243594253068231168 MS 0.175 14.77 0.74 58.8661 0.0076 208.4 5.8 0.00767 0.00059 1.042 0.079 3.93E-7 8.9E-8
27 4484348145137238016 4484348145137243904 BD 0.07 3.39 0.72 60.595 0.097 4.0 28.0 1.06 0.96 1.8 6.3 0.1 2.1
28 6082407619449932032 6082407619449930880 MS 0.560 6.04 0.31 62.295 0.050 0.07 8.8 0.07 3.8 6.0 4.4 0.8 69.0
29 2025071788687899776 2025071792959778688 WD 0.65 8.06 0.94 62.64 0.20 0.3 30.0 2.0 27.0 8.0 14.0 2.0 101.0
30 4293315765165489536 4293315662070462080 BD 0.07 9.8 2.1 65.727 0.051 79.0 76.0 0.0059 0.0059 1.19 1.2 2.3E-6 8.8E-6

Notes. The table lists the Gaia Source ID of lens and background star, the stellar type (ST) of the lens, its mass (M), the Einstein radius θE, the Julian year T after 2000 of the closest approach, with uncertainty, the minimum separation (dmin), as well as the expected shift of the combined centre of light (δθc,  lum), the shift of the brightest image only (δθ+), and the expected magnification (Δm). The corresponding errors are indicated by σ. The online table (http://dc.zah.uni-heidelberg.de/amlensing/q2/q/form) will also list positions, proper motions, parallaxes, and magnitudes for the source and lens stars, the timescale, the impact parameter in units of Einstein radii, the expected shift of the centre of light assuming a dark lens, as well as the predicted values as seen from L2. For the background source of event #2, only a two-parameter solution exists. Events #3 and #4 (light grey) are the photometric events in 2019. Event #10 (dark grey) is the event of Barnard’s star in 2035.

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