Title: 3-D selection of 167 sub-stellar companions to nearby stars Authors: Feng F., Butler R.P., Vogt S.S., Clement M.S., Tinney C.G., Cui K., Aizawa M., Jones H.R.A., Bailey J., Burt J., Carter B.D., Crane J.D., Flammini Dotti F., Holden B., Ma B., Ogihara M., Oppenheimer R., O'Toole S.J., Shectman S.A., Wittenmyer R.A., Wang S.X., Wright D.J., Xuan Y. Table: Mean separation and base-10 logarithmic flux ratio of companions to host stars ================================================================================ Byte-by-byte Description of file: apjsac7e57t5_mrt.txt -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- Companion Companion Name 14- 14 A1 --- ImFlag Direct imaging flag (1) 16- 19 I4 mas Sep Mean Separation, milliarcseconds (2) 21- 24 F4.1 [-] J0.1 Contrast, J-band, 0.1 Gyr (3) 26- 29 F4.1 [-] H0.1 Contrast, H-band, 0.1 Gyr (3) 31- 34 F4.1 [-] K0.1 Contrast, K-band, 0.1 Gyr (3) 36- 39 F4.1 [-] J1 Contrast, J-band, 1 Gyr (3) 41- 44 F4.1 [-] H1 Contrast, H-band, 1 Gyr (3) 46- 49 F4.1 [-] K1 Contrast, K-band, 1 Gyr (3) 51- 55 F5.1 [-] J10 Contrast, J-band, 10 Gyr (3) 57- 61 F5.1 [-] H10 Contrast, H-band, 10 Gyr (3) 63- 67 F5.1 [-] K10 Contrast, K-band, 10 Gyr (3) -------------------------------------------------------------------------------- Note (1): d= systems imaged and their relative astrometry data are analyzed in combination with other types of data in the solutions. Note (2): The separation of the companion to the host vary over time and the exact values for different epochs are shown in Fig. 11. Note (3): The contrasts in different bands are denoted by "BandAge" where "Band" is H, J, or K and "Age" is 0.1, 1, or 10 Gyrs. The contrast or flux ratio is in a base-10 log scale. In the calculation of the contrast of different bands, the J, H, and K magntiudes of each star are obtained from the Simbad database (Wenger et al. 2000 [2000A&AS..143....9W]), and the J, H, and K magnitudes for each companion are derived using the ATMO 2020 cooling models (Phillips et al. 2020 [2020A&A...637A..38P]) -------------------------------------------------------------------------------- GJ 2030 c 449 -4.4 -4.5 -4.6 -6.1 -6.7 -6.9 -9.2 -9.3 -10.7 GJ 3222 c 135 -2.5 -2.5 -2.4 -3.7 -3.7 -3.8 -4.9 -5.3 -5.5 GJ 680 b 1047 -2.2 -2.2 -2.3 -3.5 -4.0 -4.1 -5.4 -6.0 -6.7 GJ 864 b 298 -1.7 -1.8 -1.7 -2.8 -2.8 -2.9 -3.9 -4.4 -4.6 GJ 9714 b 601 -3.8 -4.3 -4.3 -5.6 -6.3 -6.7 -9.1 -9.0 -11.0 GJ 676 A c 609 -2.7 -2.8 -2.9 -4.7 -5.3 -5.5 -7.6 -7.9 -9.2 GJ 676 A b 109 -4.3 -4.9 -5.0 -6.7 -7.4 -7.9 -11.5 -10.8 -13.8 HD 105618 c 512 -3.6 -3.5 -3.4 -4.8 -5.2 -5.2 -6.7 -7.2 -7.8 HD 106515 A b 132 -4.4 -4.8 -4.7 -6.1 -6.8 -7.1 -9.7 -9.5 -11.4 HD 109988 b 293 -3.4 -3.3 -3.4 -4.7 -5.1 -5.2 -6.8 -7.3 -8.1 HD 110537 b 372 -3.5 -3.4 -3.3 -4.7 -5.1 -5.1 -6.5 -7.1 -7.6 HD 111031 b 420 -2.8 -2.8 -2.7 -4.0 -3.9 -4.0 -5.1 -5.5 -5.7 HD 11112 b 301 -5.0 -5.4 -5.4 -7.0 -7.6 -7.9 -10.7 -10.4 -12.6 HD 111232 c 597 -3.6 -3.6 -3.7 -5.0 -5.5 -5.6 -7.4 -7.8 -8.7 HD 113337 c 188 -4.2 -4.1 -4.1 -5.5 -5.9 -6.0 -7.8 -8.1 -8.9 HD 11505 b 519 -4.9 -5.3 -5.2 -6.8 -7.5 -7.8 -10.7 -10.3 -12.6 HD 11506 d 239 -5.1 -5.5 -5.5 -7.1 -7.8 -8.1 -11.1 -10.6 -13.0 HD 115404 A c 1034 -3.9 -4.3 -4.3 -5.7 -6.3 -6.6 -9.0 -8.9 -10.7 HD 12235 c 698 -4.8 -5.3 -5.3 -6.6 -7.3 -7.6 -10.0 -10.0 -11.8 HD 125271 b 275 -3.8 -4.3 -4.2 -5.5 -6.2 -6.5 -8.8 -8.8 -10.4 HD 127506 c 153 -2.3 -2.2 -2.2 -3.4 -3.5 -3.6 -4.7 -5.1 -5.4 HD 131509 b 641 -3.3 -3.3 -3.2 -4.4 -4.3 -4.3 -5.4 -5.9 -6.0 HD 13724 b d 286 -3.1 -3.0 -2.9 -4.3 -4.5 -4.5 -5.8 -6.2 -6.6 HD 139189 b 243 -2.7 -2.6 -2.5 -3.8 -4.1 -4.1 -5.3 -5.8 -6.1 HD 140901 c 487 -4.9 -5.4 -5.4 -7.2 -7.8 -8.3 -11.4 -10.9 -13.6 HD142 A c 375 -4.7 -4.9 -4.9 -6.4 -6.9 -7.2 -9.6 -9.5 -11.1 HD 145675 c 666 -5.2 -5.7 -5.8 -7.8 -8.3 -8.9 -13.0 -12.1 -15.1 HD 145675 b 155 -4.6 -5.0 -5.0 -6.6 -7.2 -7.6 -10.4 -10.0 -12.3 HD 149782 b 105 -2.7 -2.6 -2.5 -3.8 -3.8 -3.9 -5.0 -5.4 -5.6 HD 149806 b 610 -3.6 -3.8 -3.8 -5.3 -5.9 -6.0 -8.4 -8.5 -9.9 HD 151450 c 323 -5.4 -5.9 -6.0 -8.0 -8.5 -9.0 -13.3 -12.3 -15.3 HD 153557 d 1196 -2.9 -2.9 -2.8 -4.1 -4.6 -4.6 -5.9 -6.5 -7.1 HD 155918 c 477 -5.1 -5.6 -5.6 -7.5 -8.0 -8.5 -12.1 -11.4 -14.2 HD 156098 c 174 -5.7 -6.1 -6.1 -7.7 -8.3 -8.7 -11.5 -11.1 -13.5 HD 156279 c 152 -4.3 -4.8 -4.7 -6.1 -6.8 -7.1 -9.6 -9.4 -11.3 HD 167665 b 182 -3.0 -2.9 -2.8 -4.1 -4.1 -4.2 -5.3 -5.7 -5.9 HD 168769 b 148 -2.4 -2.3 -2.2 -3.4 -3.3 -3.4 -4.5 -4.9 -5.0 HD 168863 b 274 -4.5 -5.1 -5.0 -6.7 -7.4 -7.8 -10.9 -10.4 -13.0 HD 16905 b 162 -4.1 -4.6 -4.6 -6.0 -6.7 -7.0 -9.6 -9.4 -11.4 HD 181234 b 154 -4.6 -5.0 -5.0 -6.6 -7.2 -7.6 -10.3 -10.0 -12.2 HD 18143 c 779 -3.8 -4.3 -4.3 -5.6 -6.3 -6.6 -9.0 -9.0 -10.8 HD 182488 b d 1628 -2.8 -2.8 -2.7 -3.9 -4.3 -4.4 -5.4 -6.0 -6.4 HD 183263 c 102 -5.1 -5.5 -5.5 -7.3 -7.9 -8.3 -11.3 -10.8 -13.3 HD 188641 b 187 -3.9 -3.8 -3.7 -5.1 -5.5 -5.5 -6.8 -7.3 -7.8 HD 194490 b 139 -4.3 -4.7 -4.6 -6.0 -6.6 -6.8 -9.2 -9.2 -10.7 HD 204313 e 155 -3.8 -3.9 -3.9 -5.5 -6.0 -6.1 -8.2 -8.4 -9.5 HD 205158 c 150 -3.8 -3.7 -3.6 -5.0 -5.3 -5.4 -6.6 -7.1 -7.6 HD 210797 b 240 -2.4 -2.4 -2.3 -3.5 -3.6 -3.7 -4.8 -5.2 -5.4 HD 213519 c 496 -2.9 -2.8 -2.7 -4.0 -4.1 -4.2 -5.3 -5.7 -5.9 HD 219077 b 203 -5.0 -5.5 -5.3 -6.8 -7.5 -7.7 -10.3 -10.2 -12.0 HD 221420 A b 270 -4.1 -4.1 -4.2 -5.5 -5.9 -6.1 -7.7 -8.1 -9.0 HD 25015 b 167 -4.2 -4.7 -4.6 -6.0 -6.7 -7.1 -9.7 -9.5 -11.5 HD 25912 c 363 -3.8 -3.8 -3.9 -5.3 -5.8 -5.9 -7.9 -8.1 -9.2 HD 26161 b 247 -3.7 -3.5 -3.5 -4.9 -5.2 -5.2 -6.6 -7.1 -7.7 HD 27894 c 123 -4.7 -5.2 -5.2 -6.9 -7.6 -8.0 -11.1 -10.6 -13.3 HD 28185 c 336 -3.7 -3.7 -3.7 -5.1 -5.5 -5.6 -7.3 -7.7 -8.6 HD 29985 b 429 -4.6 -5.2 -5.2 -7.1 -7.7 -8.2 -12.1 -11.4 -14.3 HD 30177 c 185 -5.1 -5.6 -5.6 -7.5 -8.0 -8.5 -11.9 -11.2 -14.0 HD 39060 c d 136 -5.0 -5.3 -5.2 -6.7 -7.3 -7.5 -10.1 -9.9 -11.7 HD 39060 b d 510 -4.7 -4.9 -4.9 -6.4 -6.8 -7.0 -9.5 -9.4 -10.9 HD 39091 b d 181 -4.0 -4.2 -4.2 -5.6 -6.2 -6.4 -8.8 -8.9 -10.3 HD 4113 C d 1202 -2.8 -2.7 -2.6 -3.9 -3.9 -4.0 -5.1 -5.5 -5.6 HD 42581 d d 5022 -1.6 -1.6 -1.6 -2.6 -2.7 -2.8 -3.7 -4.2 -4.4 HD 43197 c 137 -4.7 -5.2 -5.1 -6.7 -7.4 -7.7 -10.5 -10.2 -12.5 HD 457 b 278 -3.7 -3.5 -3.5 -4.9 -5.3 -5.3 -6.7 -7.3 -7.8 HD 56957 b 105 -5.6 -6.0 -6.1 -8.0 -8.5 -9.0 -12.6 -11.8 -14.7 HD 62364 c 698 -3.8 -3.7 -3.7 -5.1 -5.4 -5.5 -7.0 -7.5 -8.1 HD 62364 b 357 -4.1 -4.1 -4.2 -5.6 -6.0 -6.2 -8.1 -8.3 -9.3 HD 62549 b 240 -4.8 -5.2 -5.2 -6.7 -7.4 -7.7 -10.4 -10.1 -12.3 HD 72659 c 269 -4.1 -4.0 -4.1 -5.5 -5.9 -6.0 -7.8 -8.1 -9.0 HD 73267 c 253 -5.1 -5.7 -5.7 -7.7 -8.2 -8.8 -13.0 -12.0 -15.1 HD 74014 b 208 -2.6 -2.5 -2.4 -3.7 -3.6 -3.6 -4.8 -5.1 -5.2 HD 75881 b 424 -3.6 -3.5 -3.4 -4.7 -5.0 -5.0 -6.2 -6.7 -7.0 HD 80275 b 216 -3.9 -3.8 -3.8 -5.0 -5.0 -5.1 -6.1 -6.5 -6.7 HD 80883 b 187 -4.9 -5.4 -5.5 -7.4 -8.0 -8.5 -12.5 -11.6 -14.6 HD 80913 b 162 -4.0 -3.9 -3.9 -5.2 -5.6 -5.7 -7.3 -7.8 -8.4 HD 85472 b 102 -4.0 -4.0 -3.8 -5.2 -5.6 -5.6 -6.8 -7.4 -7.8 HD 86065 b 394 -4.2 -4.6 -4.6 -6.0 -6.7 -7.0 -9.6 -9.4 -11.5 HD 87883 b 222 -4.9 -5.4 -5.4 -7.4 -7.9 -8.4 -12.5 -11.6 -14.6 HD 88072 b 387 -4.7 -5.2 -5.1 -6.7 -7.4 -7.7 -10.6 -10.2 -12.5 HD 93351 c 200 -3.5 -3.6 -3.6 -5.4 -5.9 -6.1 -8.4 -8.5 -9.8 HD 97037 b 213 -3.8 -3.8 -3.8 -5.2 -5.6 -5.7 -7.3 -7.8 -8.5 HD 984 b d 175 -3.2 -3.1 -2.9 -4.3 -4.5 -4.5 -5.7 -6.2 -6.4 HD 98649 b 149 -4.9 -5.4 -5.3 -7.1 -7.7 -8.1 -11.2 -10.7 -13.3 HIP 14729 b 177 -2.1 -2.1 -2.0 -3.2 -3.2 -3.3 -4.3 -4.8 -5.0 HIP 17157 b 537 -2.2 -2.3 -2.2 -3.3 -3.5 -3.7 -4.6 -5.2 -5.4 HIP 19976 c 286 -2.7 -2.7 -2.6 -3.9 -4.3 -4.4 -5.5 -6.2 -6.6 HIP 26196 b 134 -2.0 -2.0 -1.9 -3.0 -3.0 -3.1 -4.1 -4.6 -4.7 HIP 35965 b 317 -4.2 -4.7 -4.7 -6.1 -6.9 -7.2 -9.9 -9.7 -11.9 HIP 55507 b 199 -4.0 -4.6 -4.5 -5.9 -6.7 -7.1 -9.7 -9.5 -11.8 HIP 78395 b 413 -1.8 -1.8 -1.8 -2.8 -2.8 -2.8 -3.8 -4.2 -4.3 HIP 948 b 431 -3.0 -3.1 -3.2 -4.4 -4.9 -5.0 -6.6 -7.1 -7.9