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Table A.1.

Details of all 30 source–lens pairs approaching within 0.1 arcsec, ordered chronologically by the median epoch of peak magnification.

Lens DR2 id Lens G Source DR2 id Source G P(d < 1RE) (%) fmax Tmax Δt (d) Teff (K) M⋆ (M⊙)
4116504399886241792a 13.86 4116504399831319424b 18.85 19.95 2020 Jul 3–22 3554 0.16
4063191108246057472 13.65 4063191073886316928b 18.86 0.00 2021 Apr 30–May 25 3900 0.19
5901094750438455808 16.61 5901094746125412608 18.97 0.00 2022 Aug 8–19 3292 0.11
5411468169440274560c 16.61 5411468169435427328 20.19 6.07 2022 Aug 2–Oct 4 3772 0.10
5800510224109658240 17.72 5800510224109658368 20.09 0.00 2023 May 2–15 – 0.10d
5613074690219333504 16.04 5613074690220317312 20.84 0.00 2024 Sep 27–Oct 18 3834 0.14
3340477717172813568 10.10 3340477712874873344 20.50 0.00 2025 Jul 12–17 3428 0.26
2042703905028908928e 14.70 2042703900727995008 18.60 76.77 2025 Jul 20–27 3655 0.17
2030898139472914688 15.62 2030898105088410112 19.92 49.29 2025 Sep 1–16 4002 0.14
5529180853514968960f 14.77 5529180853515235072 20.64 4.66 2026 Feb 27–Apr 8 3922 0.18
5903487940560263936g 14.63 5903487940560263808 17.86 44.60 2026 May 25–Jun 7 4065 0.14
5819622622435541888 16.83 5819622622430477184 20.22 0.00 2027 Jan 14–Feb 13 3982 0.14
4114040737846721152h 15.89 4114040737803216768 20.19 7.25 2027 Mar 9–Apr 16 3400 0.15
4301535507904403712 19.09 4301535507885645312 20.19 0.89 2027 Feb 9–May 12 – 0.10a
4744453460527256448 16.91 4744453460527256576 16.79 0.00 2028 Feb 5–7 3737 0.15
318399257231042304i 17.27 318399257231042048 17.94 35.85 2028 Jul 10–27 – 0.10a
5918299904067162240j 14.91 5918299908365843840 13.90 45.93 2030 Mar 31–Apr 2 3613 0.10
2214946451667611904k 14.55 2214946455960518400 20.33 0.13 2030 Oct 31–Dec 9 4140 0.30
5191076183243196160l 16.44 5191076183240735232 19.84 4.27 2031 Jun 17–Aug 28 4306 0.17
6870168805525824384 12.95 6870168801226177408 18.93 0.00 2033 Jan 30–Feb 5 3664 0.26
5846206202262355712 16.99 5846206202256330240 20.25 5.67 2033 Jan 22–Mar 5 3296 0.09
6663600360559308672 10.74 6663600291839828096 18.00 0.00 2033 Apr 22–23 3302 0.21
2052808897922015360 16.60 2052808893622868352 18.45 0.00 2033 Jun 18–Jul 2 3836 0.15
116048577524991872m 15.46 116048577524443520 20.66 4.90 2033 Jul 23–Sep 13 3795 0.14
4111740078488465408 16.38 4111740074149205632b 20.40 5.17 2033 Jun 14–2034 Jan 5 4284 0.13
5232662289996360448n 15.57 5232662289986673536 20.45 6.03 2033 Sep 26–2034 Sep 22 3741 0.19
2934637564368867072o 15.49 2934637564369093632 20.74 8.77 2033 Aug 13–2034 Aug 11 3480 0.16
3425318817510655360p 16.15 3425318813215052288 19.35 27.96 2034 Sep 7–19 3546 0.15
4612462518451692672 16.42 4612462514156484864 17.56 0.00 2034 Nov 26–Dec 5 3783 0.15
5237644830027339904q 16.87 5237644830015225728 19.75 0.00 2035 Jul 2–2r 3670 0.12
Notes. Columns are Gaia DR2 id and G magnitude of the lens and the source, the probability of passing within an Einstein radius, the median and 68% confidence interval on the net magnification (including dilution by the lens) fmax, the 68% confidence interval on the epoch of peak magnification Tmax, the median and 68% confidence interval on the duration for which the magnification exceeds 10-4 (for MC samples in which it does so) Δt, and the effective temperature and mass of the lens. We provide alternative lens identifiers in the footnotes (marked ‘?’ where not certain).
(a)

2MASS J17392440–2327071.

(b)

Two-parameter astrometric solution only.

(c)

USNO-B1.0 0436–0183244?

(d)

Assumed.

(e)

G 207–14.

(f)

USNO-B1.0 0517–0163728?

(g)

USNO-B1.0 0421–0506943?

(h)

WISE J171513.77–243036.2.

(i)

LSPM J0146+3545.

(j)

WISE J175839.20–583931.6.

(k)

LSPM J2311+6858.

(l)

USNO-B1.0 0053–0028550.

(m)

LP 354–291.

(n)

USNO-B1.0 0212–0238785?

(o)

USNO-B1.0 0727–0162208?

(p)

2MASS J06095230+2319143.

(q)

USNO-B1.0 0259–0216569?

(r)

Lens and source have near-parallel proper motion and there is a small (∼1%) chance of passing within 1RE in 2036; DR3 will better constrain this.

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