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Table A.1
Exoplanet host stars having a common proper motion with another star. The ID of the host stars is the same as it is used in the EPE and the planet status is coded by R... published in a Refereed paper, S... Submitted to a professional journal, and C... announced by astronomers in professional Conferences. A planet status followed by the letter R in brackets means, the status on the EPE is not up-to-date and the planet detection is already published in a refereed paper. The fourth and fifth column show the proper motion listed in the catalog mentioned in the last column. For easy identification of the stellar companions in the online catalogs, the third column contains either the separation from the primary as calculated by the used online catalog or the latest separation measurement in case of published relative astrometric measurements.
| CCDM ... | Catalog of Components of Double and Multiple stars, Dommanget & Nys (2000). | ||||
| ASCC-2.5 V3 ... | All-sky Compiled Catalogue of 2.5 million stars (3rd version, 2009), Kharchenko (2001). | ||||
| HIP-2 ... | Hipparcos, the New Reduction, van Leeuwen (2008). | ||||
| Nomad-1 ... | Naval Observatory Merged Astrometric Dataset, Zacharias et al. (2004). | ||||
| UCAC-3 ... | Third U.S. Naval Observatory CCD Astrograph Catalog, Zacharias et al. (2010). | ||||
| PPMXL ... | The PPMXL catalog of positions and proper motions on the ICRS. Combining USNO-B1.0 | ||||
| and the two Micron All Sky Survey (2MASS)., Roeser et al. (2010). | |||||
| Tycho-2 ... | The Tycho-2 Catalogue of the 2.5 Million Brightest Stars, Høg et al. (2000). | ||||
| System | EPE planet status | r [″] | μαcosδ [mas / year] | μδ [mas / year] | Catalogue |
|
|
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| 11 Com A | R | 9 | −109.37 ± 1.26 | 89.25 ± 0.75 | ASCC-2.5-V3 |
| 11 Com B | – | – | −109 ± n.s. | 85 ± n.s. | CCDM |
| 16 Cyg A | – | – | −133.39 ± 0.82 | −163.08 ± 0.85 | ASCC-2.5-V3 |
| 16 Cyg B | R | 39.44 | −147.77 ± 0.85 | −158.39 ± 0.76 | ASCC-2.5-V3 |
| 16 Cyg C | – | close C component about 3.4′′ away from A, see Patience et al. (2002) | |||
| 30 Ari A | – | – | 137.66 ± 0.74 | −14.98 ± 0.91 | ASCC-2.5-V3 |
| – | A itself is a spectroscopic binary, see Guenther et al. (2009) | ||||
| 30 Ari B | R | 36.86 | 145.33 ± 1.21 | −12.86 ± 0.94 | ASCC-2.5-V3 |
| 55 Cnc A | R | – | −485.4 ± 0.9 | −234.4 ± 0.7 | Nomad-1 |
| 55 Cnc B | – | 84.16 | −488.0 ± 6.0 | −234.0 ± 5.0 | Nomad-1 |
| 91 Aqr A | S | – | 370.70 ± 0.63 | −16.22 ± 0.7 | ASCC-2.5 V3 |
| 91 Aqr B | – | 51.93 | 373.00 ± 2.41 | −18.46 ± 2.41 | ASCC-2.5 V3 |
| 91 Aqr C | – | 52.03 | 370.00 ± 1.87 | −20.34 ± 0.98 | ASCC-2.5 V3 |
| 91 Aqr D | – | 106.67 | 18.3 ± 8.4 | −10.5 ± 7.8 | Nomad-1 |
| 91 Aqr E | – | 88.05 | −9.4 ± 8.7 | −25.2 ± 7.8 | Nomad-1 |
| γ Cep A | R | – | −48.8 ± 0.4 | 127.1 ± 0.4 | Nomad-1 |
| γ Cep B | – | 0.02 | imaged directly by Neuhäuser et al. (2007) | ||
| γ1 Leo A | R | – | 306.35 ± 3.27 | −160.77 ± 2.30 | ASCC-2.5 V3 |
| γ1 Leo B | – | 4.33 | 309.60 ± 1.32 | −152.91 ± 0.75 | ASCC-2.5 V3 |
| γ1 Leo C | – | 325.15 | −501.30 ± 1.05 | −41.97 ± 1.28 | ASCC-2.5 V3 |
| γ1 Leo D | – | 366.86 | −10.01 ± 1.53 | −22.85 ± 1.21 | ASCC-2.5 V3 |
| τ Boo A | R | – | −479.53 ± 0.16 | 53.49 ± 0.13 | HIP-2 |
| τ Boo B | – | 2.8 | confirmed by Duquennoy & Mayor (1991) | ||
| υ And A | R | – | −172.5 ± 0.5 | −381.0 ± 0.4 | Nomad-1 |
| υ And B | – | 55 | confirmed by Lowrance et al. (2002) | ||
| υ And C | – | 110.27 | −9.6 ± 2.3 | −3.5 ± 2. | Nomad-1 |
| υ And D | – | 273.20 | 16.3 ± 0.7 | −4.7 ± 0.6 | Nomad-1 |
| GJ 667 AB | – | – | 1129.76 ± 9.72 | −77.02 ± 4.67 | HIP-2 |
| – | – | 1171.69 ± 2.70 | −168.80 ± 2.79 | ASCC-2.5 V3 | |
| – | – | 1161.4 ± 2.3 | −172.3 ± 2.3 | PPMXL | |
| GJ 667 C | R | 32.66 | 1049.0 ± n.s. | −91.0 ± n.s. | UCAC-3 |
| 32.75 | 1155.0 ± 7.2 | −214.4 ± 9.5 | NOMAD-1 | ||
| GJ 667 C has not a common proper motion within the measurement errors, but it can be ruled out as a background object. | |||||
| The large spread in the proper motion measurements can be possibly explained by the fact, that the AB component | |||||
| influences the relative astrometric measurements of the (AB)&C pair. | |||||
| GJ 676 A | R | – | −259.2 ± 1.4 | −185.6 ± 0.9 | Nomad-1 |
| GJ 676 B | – | 48.98 | −254.0 ± 8.0 | −156.0 ± 23.0 | Nomad-1 |
| 47.78 | −294.6 ± 7.4 | −186.8 ± 7.0 | UCAC-3 | ||
| GJ 3021 A | R | – | 433.8 ± 0.5 | −57.9 ± 0.4 | Nomad-1 |
| GJ 3021 B | – | 3.86 | confirmed by Chauvin et al. (2006) | ||
| Gl 86 A | R | – | 2183.43 ± 3.20 | 661.70 ± 3.50 | ASCC-2.5-V3 |
| Gl 86 B | – | 1.93 | confirmed by Mugrauer & Neuhäuser (2005) | ||
| HAT-P-1 A | – | – | 30.0 ± 0.6 | −42.3 ± 1.3 | UCAC-3 |
| HAT-P-1 B | R | 10.93 | 32.6 ± 0.8 | −43.2 ± 1.9 | UCAC-3 |
| WASP-8 A | S(R) | – | 109.62 ± 2.05 | 10.02 ± 1.46 | ASCC-2.5 V3 |
| WASP-8 B | – | confirmed by Queloz et al. (2010) | |||
| WASP-8 C | – | 140.93 | 50.33 ± 1.39 | −28.65 ± 1.08 | ASCC-2.5 V3 |
| XO-2 A | C(R) | – | −34.72 ± 2.50 | −153.61 ± 2.40 | ASCC-2.5 V3 |
| XO-2 B | – | 30.05 | −33.02 ± 2.89 | −154.11 ± 2.70 | ASCC-2.5 V3 |
| HD 142 A | R | – | 575.2 ± 0.4 | −39.9 ± 0.5 | Nomad-1 |
| HD 142 B | – | 4.10 | confirmed by Eggenberger et al. (2007) | ||
| HD 3651 A | R | – | −460.22 ± 0.89 | −370.22 ± 0.75 | ASCC-2.5 V3 |
| HD 3651 B | – | 43.07 | confirmed by Mugrauer et al. (2006b) | ||
| HD 3651 C | – | 168.26 | 10.81 ± 2.00 | −1.48 ± 2.40 | ASCC-2.5 V3 |
| HD 7449 A | R | – | −161.6 ± 0.6 | −138.9 ± 0.5 | PPMXL |
| HD 7449 B | 60.20 | −162.5 ± 6.1 | −137.5 ± 6.1 | PPMXL | |
| HD 16141 A | R | – | −155.33 ± 1.19 | −437.42 ± 1.23 | ASCC-2.5 V3 |
| HD 16141 B | – | 6.20 | confirmed by Mugrauer et al. (2005) | ||
| HD 11964 A | R | – | −366.10 ± 0.3 | −240.83 ± 0.62 | ASCC-2.5 V3 |
| HD 11964 B | – | 30.68 | −369.98 ± 4.34 | −245.47 ± 3.13 | ASCC-2.5 V3 |
| HD 19994 A | R | – | 194.56 ± 0.37 | −69.01 ± 0.30 | HIP-2 |
| HD 19994 BC | – | 2.30 | confirmed by Duquennoy & Mayor (1991) | ||
| close C component around B found by Roell et al. (2011) | |||||
| HD 20782 A | R | – | 349.85 ± 0.80 | −65.00 ± 1.07 | ASCC-2.5 V3 |
| HD 20782 B | – | 253.71 | 349.76 ± 1.13 | −68.44 ± 1.57 | ASCC-2.5 V3 |
| HD 27442 A | R | – | −48.09 ± 0.80 | −166.69 ± 0.77 | ASCC-2.5 V3 |
| HD 27442 B | – | 13.06 | confirmed by Chauvin et al. (2006) | ||
| HD 28254 A | S(R) | – | −66.9 ± 0.6 | −144.0 ± 0.6 | Nomad-1 |
| HD 28254 B | – | 4.3 | confirmed by Naef et al. (2010) | ||
| HD 38529 A | R | – | −79.22 ± 1.02 | −142.22 ± 1.00 | ASCC-2.5 V3 |
| HD 38529 B | – | 283.72 | −81.79 ± 14.50 | −117.47 ± 14.80 | ASCC-2.5 V3 |
| B component confirmed by Raghavan et al. (2006) | |||||
| HD 40979 A | R | – | 96.40 ± 1.19 | −153.36 ± 0.70 | ASCC-2.5 V3 |
| HD 40979 BC | – | 193.77 | 94.08 ± 1.85 | −153.11 ± 1.65 | ASCC-2.5 V3 |
| – | C component about 3.9′′ away from B found by Mugrauer et al. (2007a) | ||||
| HD 41004 A | R | – | −41.72 ± 1.19 | 64.87 ± 1.34 | ASCC-2.5 V3 |
| HD 41004 B | R | 1.19 | −42.25 ± 1.08 | 65.16 ± 1.12 | ASCC-2.5 V3 |
| HD 46375 A | R | – | 114.2 ± 0.9 | −96.7 ± 0.7 | Nomad-1 |
| HD 46375 B | 10.35 | confirmed by Mugrauer et al. (2006a) | |||
| HD 65216 A | R | – | −122.66 ± 1.34 | 145.77 ± 1.15 | ASCC-2.5 V3 |
| HD 65216 BC | – | 7.14 | confirmed by Mugrauer et al. (2007b) | ||
| C component 0.17′′ away from B found by Mugrauer et al. (2007b) | |||||
| HD 75289 A | R | – | −19.90 ± 0.66 | −228.13 ± 0.73 | ASCC-2.5 V3 |
| HD 75289 B | – | 21.47 | confirmed by Mugrauer et al. (2004a) | ||
| HD 80606 A | R | – | 56.84 ± 1.37 | 10.02 ± 1.71 | ASCC-2.5 V3 |
| HD 80606 B | 20.18 | 51.95 ± 1.32 | 9.97 ± 1.77 | ASCC-2.5 V3 | |
| HD 89744 A | R | – | −120.12 ± 0.85 | −138.66 ± 0.76 | ASCC-2.5 V3 |
| HD 89744 B | – | 62.99 | confirmed by Mugrauer et al. (2004b) | ||
| HD 99491 (A) | – | – | −725.22 ± 0.64 | 180.30 ± 0.72 | ASCC-2.5 V3 |
| HD 99492 (B) | R | 33.27 | −727.57 ± 1.55 | 186.47 ± 1.55 | ASCC-2.5 V3 |
| HD 99492 (C) | – | 204.56 | 5.36 ± 1.98 | −13.72 ± 2.00 | ASCC-2.5 V3 |
| HD 101930 A | R | – | 15.42 ± 1.30 | 348.29 ± 1.27 | ASCC-2.5 V3 |
| HD 101930 B | – | 69.89 | 24.98 ± 4.01 | 351.54 ± 2.35 | ASCC-2.5 V3 |
| – | B component confirmed by Mugrauer et al. (2007b) | ||||
| HD 109749 A | C(R) | – | −156.69 ± 1.47 | −4.88 ± 1.54 | ASCC-2.5 V3 |
| HD 109749 B | – | 8.42 | −157.88 ± 1.42 | −5.46 ± 1.28 | ASCC-2.5 V3 |
| HD 114729 A | R | – | −200.83 ± 1.23 | −307.82 ± 1.11 | ASCC-2.5 V3 |
| HD 114729 B | – | 8.05 | confirmed by Mugrauer et al. (2005) | ||
| HD 114762 A | R | – | −582.75 ± 1.12 | −1.04 ± 1.07 | ASCC-2.5 V3 |
| HD 114762 B | – | 3.26 | confirmed by Patience et al. (2002) | ||
| HD 125612 A | S(R) | – | −62.25 ± 1.66 | −67.63 ± 1.50 | ASCC-2.5 V3 |
| HD 125612 B | – | 89.99 | confirmed by Mugrauer & Neuhäuser (2009) | ||
| HD 126614 AB | S(R) | – | −151.66 ± 1.35 | −148.66 ± 1.22 | ASCC-2.5 V3 |
| – | −152.4 ± 1.0 | −148.1 ± 0.9 | Nomad-1 | ||
| B is 0.5′′ away from A, found by Howard et al. (2010) | |||||
| and common proper motion confirmed by Ginski et al. (2012) | |||||
| HD 126614 C | – | 41.80 | −144.0 ± 4.0 | −142.0 ± 3.0 | Nomad-1 |
| HD 132563 A | – | – | −56.38 ± 2.22 | −68.87 ± 1.69 | ASCC-2.5 V3 |
| A itself is a spectroscopic binary, see Desidera et al. (2011) | |||||
| HD 132563 B | R | 3.79 | −57.15 ± 2.11 | −69.18 ± 1.62 | ASCC-2.5 V3 |
| HD 132563 C | – | 64.77 | −14.52 ± 1.57 | 7.36 ± 1.02 | ASCC-2.5 V3 |
| HD 137388 A | R | – | −46.72 ± 0.89 | 43.31 ± 0.97 | HIP-2 |
| HD 137388 B | – | 21.31 | −35.54 ± 14.33 | 74.43 ± 16.63 | HIP-2 |
| – | 21.32 | −94.69 ± 58.77 | 38.04 ± 63.18 | ASCC-2.5 V3 | |
| HD 142022 A | R | – | −340.52 ± 0.91 | −31.04 ± 1.01 | ASCC-2.5 V3 |
| HD 142022 B | – | 22.85 | −359.70 ± 2.38 | −26.28 ± 2.04 | ASCC-2.5 V3 |
| HD 147513 A | R | – | 72.47 ± 0.93 | 3.43 ± 0.83 | ASCC-2.5 V3 |
| HD 147513 B | – | 345.69 | 76.73 ± 2.17 | 1.94 ± 2.10 | ASCC-2.5 V3 |
| HD 177830 A | R | – | −40.83 ± 0.75 | −50.13 ± 0.99 | ASCC-2.5 V3 |
| HD 177830 B | – | 1.65 | confirmed by Eggenberger et al. (2007) | ||
| HD 178911 A | – | – | 50.20 ± 1.87 | 190.05 ± 2.46 | ASCC-2.5 V3 |
| – | 51.89 ± 2.09 | 196.24 ± 2.31 | HIP-2 | ||
| – | A itself is a spectroscopic binary, see McAlister et al. (1987) | ||||
| HD 178911 B | R | 16.86 | 67.13 ± 2.11 | 190.50 ± 2.64 | ASCC-2.5 V3 |
| 16.85 | 55.14 ± 3.43 | 201.30 ± 4.39 | HIP-2 | ||
| HD 185269 A | R | – | −32.3 ± 0.5 | −80.7 ± 0.6 | PPMXL |
| HD 185269 B | – | 4.51 | confirmed by Ginski et al. (2012) | ||
| HD 188015 A | R | – | 55.61 ± 0.12 | −91.62 ± 1.11 | ASCC-2.5 V3 |
| HD 188015 B | – | 13 | confirmed by Raghavan et al. (2006) | ||
| HD 189733 A | R | – | −2.39 ± 0.87 | −250.19 ± 0.80 | ASCC-2.5 V3 |
| HD 189733 B | – | 11.37 | confirmed by Bakos et al. (2006) | ||
| HD 190360 A | R | – | 683.3 ± 0.4 | −524.0 ± 0.5 | Nomad-1 |
| HD 190360 B | – | 178.00 | 686.8 ± 4.1 | −530.3 ± 4.1 | Nomad-1 |
| HD 195019 A | R | – | 349.54 ± 1.12 | −57.27 ± 0.82 | ASCC-2.5 V3 |
| HD 195019 B | – | Multiplicity first mentioned by Fischer et al. (1999) | |||
| HD 196050 A | R | – | −191.30 ± 0.85 | −63.31 ± 0.99 | ASCC-2.5 V3 |
| HD 196050 BC | – | 10.88 | confirmed by Mugrauer et al. (2005) | ||
| – | C component about 0.4′′ away from B found by Eggenberger et al. (2007) | ||||
| HD 196885 A | R | – | 47.4 ± 0.8 | 83.0 ± 0.5 | Nomad-1 |
| – | 56.5 ± 1.1 | 87.3 ± 1.2 | Tycho-2 | ||
| HD 196885 B | – | 0.70 | confirmed by Chauvin et al. (2011) | ||
| HD 196885 C | – | 183.06 | −5.2 ± 1.4 | −3.9 ± 1.3 | Nomad-1 |
| – | 183.12 | −3.1 ± 1.5 | −2.2 ± 1.4 | Tycho-2 | |
| HD 204941 A | R | – | −298.24 ± 1.34 | −124.68 ± 0.67 | ASCC-2.5 V3 |
| HD 204941 B | – | 53.62 | −308.85 ± 3.48 | −124.13 ± 1.84 | ASCC-2.5 V3 |
| HD 212301 A | S(R) | – | 79.12 ± 1.04 | −92.37 ± 0.99 | ASCC-2.5 V3 |
| HD 212301 B | – | 4.43 | confirmed by Mugrauer & Neuhäuser (2009) | ||
| HD 213240 A | R | – | −135.1 ± 0.6 | −194.0 ± 0.4 | Nomad-1 |
| HD 213240 B | – | 21.94 | 65.1 ± 5.0 | −10.8 ± 1.5 | Nomad-1 |
| HD 213240 C | – | 95.69 | confirmed by Mugrauer et al. (2005) | ||
| HD 222582 A | R | – | −145.4 ± 1.2 | −111.0 ± 0.8 | Nomad-1 |
| HD 222582 B | – | 109.42 | −147.5 ± 4.4 | −114.2 ± 4.4 | Nomad-1 |
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