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Table A.1

Detected companions in the sample of stars observed with AstraLux presented in this work. The main target is labelled with an “A” in the ID column, AstraLux-detected companions are labelled with a “B,” and other Gaia sources are labelled “Gaia.”

TOI ID sep PA ∆mSDSSz Gaia DR3 counterpart d μα μδ
(arcsec) (deg.) (mag) (pc) (mas/yr) (mas/yr)
TOI-498 A - - - 3071584413361857280 192.1 ± 1.6 -21.69 4.02
B 2.1792 ± 0.0029 106.82 ± 0.18 3.355 ± 0.024 3071584417657701504 5480 ± 910 2.74 -2.57

TOI-676 A - - - 3546125626089939968 709 ± 11 -20.85 9.13
B 1.4726 ± 0.0087 98.1 ± 1.5 3.42 ± 0.23 3546125630386919424 590 ± 23 -20.76 8.73

TOI-680 A - - - 3574891599052022144 160.1 ± 1.7 -56.67 -6.57
B 0.7679 ± 0.0045 26.59 ± 0.14 3.690 ± 0.042 - - - -

TOI-1001 A - - - 3067555424799970560 287.5 ± 1.5 -4.92 -15.43
B 1.5541 ± 0.0066 −1.43 ± 0.14 5.030 ± 0.075 3067555429095077376 - - -

TOI-1169 A - - - 1122163457093871744 258.50 ± 0.97 -5.67 7.79
B 1.6507 ± 0.0030 -5.840 ± 0.062 1.285 ± 0.039 1122163461390307072 - - -
Gaia 1.67 -13.8 0.7 1122163461390307072 257.3 ± 1.2 -3.91 7.99

TOI-1201 A - - - 5157183324996790272 37.636 ± 0.032 164.07 46.55
B 8.2994 ± 0.0017 -99.310 ± 0.032 1.505 ± 0.036 5157183324996789760 37.680 ± 0.033 174.43 45.46

TOI-1242 A - - - 1624420987137541376 109.52 ± 0.16 1.64 -39.84
B 4.3836 ± 0.0048 3.776 ± 0.030 2.855 ± 0.050 1624420991433145472 109 ± 22 1.84 -39.60

TOI-1261†† A - - - 1417009251113227648 199.90 ± 0.44 -4.12 18.08
B 1.6346 ± 0.0041 42.088 ± 0.070 2.685 ± 0.037 1417009255408193536 - - -
Gaia 2.29 57.52 3.2 1417009255408193536 201.2 ± 1.4 -3.32 17.07

TOI-1280 A - - - 2240116441786134912 92.325 ± 0.080 19.18 -23.27
B 6.2683 ± 0.0018 88.02 ± 0.19 -1.230 ± 0.029 2240116441786135680 672.3 ± 9.0 -6.35 -8.84

TOI-1293†† A - - - 1640813919530112512 236.58 ± 0.91 20.73 -37.98
B 0.8897 ± 0.0067 236.57 ± 0.29 4.52 ± 0.15 1640813919529592448 - - -
Gaia 2.32 253.6 4.7 1640813919529592448 - - -

TOI-1297†† A - - - 1679498552524609664 455 ± 16 -14.03 4.89
B 0.6333 ± 0.0068 66.10 ± 0.57 2.15 ± 0.11 1679498552525334656 - - -
Gaia 1.66 82.25 0.36 1679498552525334656 456 ± 25 -13.77 6.88

TOI-1331 A - - - 2171356454931124864 400.2 ± 1.9 0.4 -13.16
B 4.1999 ± 0.0016 −68.090 ± 0.049 2.380 ± 0.019 2171356454931124992 657.9 ± 5.5 -1.64 2.97

TOI-1450†† A - - - 2155540255030594560 22.4425 ± 0.0079 69.99 160.8
B 3.1709 ± 0.0032 36.305 ± 0.025 3.753 ± 0.036 2155540255030594688 - - -
Gaia 4.77 124.9 3.8 2155540255030594688 22.461 ± 0.013 83.3 143.8

TOI-1452 A - - - 2264839957167921024 30.504 ± 0.013 7.8 -74.08
B 3.0900 ± 0.0015 −3.162 ± 0.016 0.483 ± 0.016 2264839952875245696 30.496 ± 0.013 6.85 -82.22

TOI-1453†† A - - - 1433062331332673792 78.887 ± 0.064 -70.97 -0.09
B 1.8503 ± 0.0064 56.04 ± 0.12 4.354 ± 0.066 1433062331333157632 - - -
Gaia 3.02 110.7 5.2 1433062331333157632 78.53 ± 0.42 74.8 2.3

TOI-1654†† A - - - 2255021730651241728 292.6 ± 1.9 6.02 -19.17
B 1.0360 ± 0.0019 81.33 ± 0.25 0.938 ± 0.017 2255021730648557184 - - -
Gaia 2.6 86.9 0.81 2255021730648557184 284.7 ± 2.6 4.8 -18.9

TOI-2072 A - - - 1079565834014085632 39.018 ± 0.029 -184.97 -87.24
B 2.9558 ± 0.0018 −134.667 ± 0.018 1.068 ± 0.020 - - - -
Gaia 9.3 102 0.92 1079565834013188864 39.132 ± 0.029 -184.6 -92.0

TOI-5128 A - - - 588253843440407808 192.9 ± 1.2 -17.34 -14.67
B 1.4238 ± 0.0012 3.808 ± 0.023 2.324 ± 0.011 588253843440048768 203.5 ± 1.9 -18.25 -14.39

TOI-5377 A - - - 1040790426885870976 268 ± 40 -37.62 -53.21
B 0.1975 ± 0.0013 57.44 ± 0.28 0.6845 ± 0.0099 - - - -

TOI-5474 A - - - 3450525873195051136 710.3 ± 7.1 -0.6 -7.67
B 1.3339 ± 0.0036 101.32 ± 0.55 2.395 ± 0.046 3450525877490978176 - - -
Gaia 1.65 98.57 1.83 3450525877490978176 - - -

Notes. (†)Companions detected by AstraLux are also confidently detected with Gaia DR3, and their proper motions and distances point to them being physically bound to the main target. (††)The companions detected by AstraLux do not fully match the position of a nearby Gaia DR3 source that is likely physically bound to the main target. This can either be because the AstraLux detection corresponds to another source or because we are detecting the binary orbital motion of the Gaia source (see, e.g., the case of TOI-1450). (‡)Gaia DR3 source ID to which the source could potentially be associated.

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