Target . | Distance . | Distance . | π errora . | a(col)b . | rms(col)c . | error(col)d . | |$\epsilon _i\, ^e$| . | |$D\, ^f$| . | RUWEg . | Matched . |
---|---|---|---|---|---|---|---|---|---|---|
. | This work (pc) . | Gaia (pc) . | (μas) . | (μas) . | (μas) . | (μas) . | (μas) . | ... . | ... . | transits . |
37743815 | 1789 ± 78 | 1857 ± 39 | 11 | 119 | 104 | 15 | 35 | 1.20 | 1.09 | 54 |
42565581 | 3150 ± 150 | 3281 ± 160 | 15 | 63 | 47 | 11 | 39 | 1.04 | 1.17 | 24 |
54060695 | 2427 ± 34 | 2221 ± 50 | 10 | 80 | 57 | 7 | 37 | 2.26 | 0.94 | 67 |
178010808 | 1415 ± 22 | 1464 ± 30 | 13 | 90 | 73 | 10 | 56 | 5.14 | 1.04 | 59 |
242132789 | 2667 ± 28 | 3258 ± 165 | 16 | 73 | 52 | 9 | 32 | 0.82 | 1.10 | 37 |
456194776 | 1690 ± 24 | 1590 ± 40 | 16 | 159 | 130 | 20 | 52 | 4.46 | 0.95 | 49 |
Target . | Distance . | Distance . | π errora . | a(col)b . | rms(col)c . | error(col)d . | |$\epsilon _i\, ^e$| . | |$D\, ^f$| . | RUWEg . | Matched . |
---|---|---|---|---|---|---|---|---|---|---|
. | This work (pc) . | Gaia (pc) . | (μas) . | (μas) . | (μas) . | (μas) . | (μas) . | ... . | ... . | transits . |
37743815 | 1789 ± 78 | 1857 ± 39 | 11 | 119 | 104 | 15 | 35 | 1.20 | 1.09 | 54 |
42565581 | 3150 ± 150 | 3281 ± 160 | 15 | 63 | 47 | 11 | 39 | 1.04 | 1.17 | 24 |
54060695 | 2427 ± 34 | 2221 ± 50 | 10 | 80 | 57 | 7 | 37 | 2.26 | 0.94 | 67 |
178010808 | 1415 ± 22 | 1464 ± 30 | 13 | 90 | 73 | 10 | 56 | 5.14 | 1.04 | 59 |
242132789 | 2667 ± 28 | 3258 ± 165 | 16 | 73 | 52 | 9 | 32 | 0.82 | 1.10 | 37 |
456194776 | 1690 ± 24 | 1590 ± 40 | 16 | 159 | 130 | 20 | 52 | 4.46 | 0.95 | 49 |
Note. (a) Gaia uncertainty in the parallax (parallax_error). (b) Semimajor axis of the triple’s centre of light (‘col’) expressed in micro-arc seconds. (c) RMS fluctuations due to the triple’s centre of light motion. (d) Error contribution due to the triple’s centre of light motion (see the text). (e) Gaia’s astrometric_excess_noise. (f) Gaia’s astrometric_excess_noise_significance. (g) Gaia’s renormalized unit weight error – RUWE parameter. (h) The number of astrometric_matched_transits.
Target . | Distance . | Distance . | π errora . | a(col)b . | rms(col)c . | error(col)d . | |$\epsilon _i\, ^e$| . | |$D\, ^f$| . | RUWEg . | Matched . |
---|---|---|---|---|---|---|---|---|---|---|
. | This work (pc) . | Gaia (pc) . | (μas) . | (μas) . | (μas) . | (μas) . | (μas) . | ... . | ... . | transits . |
37743815 | 1789 ± 78 | 1857 ± 39 | 11 | 119 | 104 | 15 | 35 | 1.20 | 1.09 | 54 |
42565581 | 3150 ± 150 | 3281 ± 160 | 15 | 63 | 47 | 11 | 39 | 1.04 | 1.17 | 24 |
54060695 | 2427 ± 34 | 2221 ± 50 | 10 | 80 | 57 | 7 | 37 | 2.26 | 0.94 | 67 |
178010808 | 1415 ± 22 | 1464 ± 30 | 13 | 90 | 73 | 10 | 56 | 5.14 | 1.04 | 59 |
242132789 | 2667 ± 28 | 3258 ± 165 | 16 | 73 | 52 | 9 | 32 | 0.82 | 1.10 | 37 |
456194776 | 1690 ± 24 | 1590 ± 40 | 16 | 159 | 130 | 20 | 52 | 4.46 | 0.95 | 49 |
Target . | Distance . | Distance . | π errora . | a(col)b . | rms(col)c . | error(col)d . | |$\epsilon _i\, ^e$| . | |$D\, ^f$| . | RUWEg . | Matched . |
---|---|---|---|---|---|---|---|---|---|---|
. | This work (pc) . | Gaia (pc) . | (μas) . | (μas) . | (μas) . | (μas) . | (μas) . | ... . | ... . | transits . |
37743815 | 1789 ± 78 | 1857 ± 39 | 11 | 119 | 104 | 15 | 35 | 1.20 | 1.09 | 54 |
42565581 | 3150 ± 150 | 3281 ± 160 | 15 | 63 | 47 | 11 | 39 | 1.04 | 1.17 | 24 |
54060695 | 2427 ± 34 | 2221 ± 50 | 10 | 80 | 57 | 7 | 37 | 2.26 | 0.94 | 67 |
178010808 | 1415 ± 22 | 1464 ± 30 | 13 | 90 | 73 | 10 | 56 | 5.14 | 1.04 | 59 |
242132789 | 2667 ± 28 | 3258 ± 165 | 16 | 73 | 52 | 9 | 32 | 0.82 | 1.10 | 37 |
456194776 | 1690 ± 24 | 1590 ± 40 | 16 | 159 | 130 | 20 | 52 | 4.46 | 0.95 | 49 |
Note. (a) Gaia uncertainty in the parallax (parallax_error). (b) Semimajor axis of the triple’s centre of light (‘col’) expressed in micro-arc seconds. (c) RMS fluctuations due to the triple’s centre of light motion. (d) Error contribution due to the triple’s centre of light motion (see the text). (e) Gaia’s astrometric_excess_noise. (f) Gaia’s astrometric_excess_noise_significance. (g) Gaia’s renormalized unit weight error – RUWE parameter. (h) The number of astrometric_matched_transits.
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