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Table D.1

Input catalogue with the main planetary and stellar properties for the confirmed exoplanets that are Roman-accessible.

Planet d P a Mp Rp i e ωp T St. type M V Age
[pc] [days] [AU] [MJ] [RJ] [deg] [deg] K [M] [mag] [Gyr]
GJ 687 c 4.55 727.6 1.17 0.050 (†) 0.40 356.0 3826 M3 V 0.40 9.150
55 Cnc d 12.59 4825.0 5.50 3.878 (†) 90.0 0.02 224.0 5196 G8 V 0.91 5.960 10.20
HD 114613 b 20.29 4000.0 5.34 0.357 (†) 0.46 16.0 5641 G4 IV 1.27 4.850
ups And d 13.41 1276.5 2.51 4.132 (†) 0.30 78.8 6105 F8 V 1.30 4.100 5.00
HD 217107 c 20.07 4270.0 5.32 2.600 (†) 0.52 18.6 5622 G8 IV 1.00 6.160
GJ 179 b 12.36 2288.0 2.41 0.820 (†) 0.21 333.0 3370 M3.5 V 0.36 12.000
14 Her b 17.94 1773.4 2.93 4.660 (†) 0.37 5338 K0 V 0.90 6.610
47 UMa c 13.80 2391.0 3.60 0.540 (†) 0.10 115.0 5892 G0 V 1.03 5.050 7.30
47 UMa b 13.80 1078.0 2.10 2.530 (†) 0.03 154.0 5892 G0 V 1.03 5.050 7.30
GJ 9066 c 4.47 767.9 0.87 0.225 (†) 0.33 98.0 3305 M4.5 V 0.15 12.270
pi Men b 18.28 2093.1 3.10 10.020 (†) 0.64 150.6 6037 G0 V 1.09 5.670 2.98
HD 190360 b 16.01 2915.0 3.97 1.540 (†) 0.31 5552 G6 IV 0.99 5.730
GJ 229 b 5.76 526.1 0.90 0.027 (†) 0.10 19.0 3913 M1/M2 V 0.58 8.140
GJ 328 b 20.54 4100.0 4.50 2.300 (†) 0.37 110.0 3900 M1 0.69 9.970
psi 1 Dra B b 22.16 3117.0 4.43 1.530 (†) 0.40 244.0 6212 G0 V 1.19 5.699 3.30
GJ 849 b 8.80 1882.0 2.35 1.000 (†) 0.04 3241 M3 V 0.65 10.370
HD 154345 b 18.29 3341.6 4.21 0.820 (†) 0.04 5468 G8 V 0.71 6.760
RR Cae b 21.20 4343.5 5.30 4.200 (†) 90.0 0.00 4134 M 0.44
HD 87883 b 18.30 2754.0 3.58 1.540 (†) 0.53 4915 K2.5 V 0.66 7.550
HIP 38594 c 17.80 3477.8 3.81 0.152 (†) 0.16 16.0 4086 M0 0.61 9.770
HD 114783 c 20.40 4319.0 0.611 (†) 0.00 186.5 5135 K0 0.85 7.550
HD 219077 b 29.21 5501.0 6.22 10.390 (†) 0.77 237.6 5362 G8 V 1.05 6.120 8.90
HD 134987 c 26.20 5000.0 5.80 0.820 (†) 0.12 15.0 5736 G5 V 1.10 6.450
GJ 317 c 15.10 6739.3 5.23 1.644 (†) 0.17 288.0 3590 M2.5 V 0.42 11.970
HD 160691 c 15.61 4205.8 5.24 1.814 (†) 0.10 237.6 5804 G5 V 1.08 5.150 6.40
HD 113538 c 15.90 1818.0 2.44 0.930 (†) 0.20 100.0 4462 K9 V 0.58 9.057 4.30
HD 219134 h 6.53 2247.0 3.11 0.340 (†) 0.06 35.0 4699 K3 V 0.81 5.570 11.00
HD 142 c 26.21 6005.0 6.80 5.300 (†) 0.21 70.0 6245 G1 IV 1.23 5.700
HD 106515 A b 34.12 3630.0 4.59 9.610 (†) 0.57 303.8 5362 G5 0.97 7.972 11.70
gam Cep b 13.54 903.3 2.05 1.850 (†) 0.05 274.6 4707 K1 IV 1.40 3.210
HD 65216 c 35.16 5370.0 5.75 2.030 (†) 0.17 303.0 5612 G5 V 0.87 7.964
HAT-P-11 c 37.81 3407.0 4.13 1.595 (†) 0.60 323.7 4780 K4 0.81 9.174 6.50
GJ 676 A c 16.03 7337.0 6.60 6.800 (†) 3734 M0 V 0.73 9.580
HR 5183 b 31.49 27 000.0 18.00 3.230 (†) 0.84 160.0 5794 G0 V 1.07 6.300 7.70
HD 181433 d 26.90 2172.0 3.00 0.540(†) 0.48 150.0 4918 K3 IV 0.63 8.400
tau Cet e 3.60 162.9 0.54 0.012 (†) 0.18 202.3 5375 G8 V 0.78 3.500
HD 92788 c 34.69 11 611.3 10.50 3.670 (†) 0.46 154.3 5744 G6 V 1.15 7.310 2.55
bet Pic c 19.75 1230.0 2.72 8.200 1.20 89.2 0.37 66.2 7100 A5 V 1.76 3.850
DE CVn b 30.55 4098.1 5.75 12.029 86.0 0.00 3586 0.51
HD 62509 b 10.34 589.6 1.64 2.300 (†) 0.02 174.6 4946 K0 III 2.10 1.140 0.98
HD 100546 b 110.02 53.00 6.90 10 500 B9 Vne 2.40 6.704 0.01
HD 141399 e 36.20 5000.0 5.00 0.660 (†) 0.26 170.0 5600 K0 1.07 7.200
2MASS J21+16 b (a) 25.00 7336.5 20.950 0.92 46.2 0.26 43.0 2300 M8.5 0.08
GJ 433 c 9.07 5094.1 4.82 0.102 (†) 0.12 62.0 3781 M1.5 V 0.48 9.806
WISEP J12+16 b (b) 10.10 8.00 22.000 0.93 575 T8.5 0.03 6.00
GJ 832 b 4.97 3657.0 3.56 0.680 (†) 0.08 66.0 3472 M1.5 0.45 8.660
HD 150706 b 28.29 5894.0 6.70 2.710 (†) 0.38 312.0 5961 G0 V 1.17 7.020 3.00
eps Eri b 3.22 2690.0 0.780 89.0 0.07 355.0 4975 K2 V 0.78 3.820 0.50
Wolf 1061 d 4.31 217.2 0.47 0.024 (†) 0.55 3342 M3.5 0.29 10.030
HIP 70849 b 24.07 17 337.5 20.25 9.000 (†) 0.71 4105 K7 V 0.63 10.360 3.00
HD 192310 c 8.80 525.8 1.18 0.076 (†) 0.32 290.0 5166 K3 V 0.80 5.730 7.81
HD 25015 b 37.47 6019.3 6.19 4.480 (†) 0.39 257.7 5160 K1 V 0.86 8.870 4.00
CFBDSIR J14+10 b (c) 23.10 10 037.5 2.60 10.500 580 0.02
HD 30562 b 26.18 1157.0 2.34 1.220 (†) 0.76 5882 F8 V 1.12 5.780
GJ 15 A c 3.56 7600.0 5.40 0.113 (†) 0.27 121.6 3607 M1 0.38 8.080
tau Cet f 3.60 636.1 1.33 0.012 (†) 0.16 299.8 5375 G8 V 0.78 3.500
GJ 676 A b 16.03 1056.8 1.82 4.960 (†) 0.33 3734 M0 V 0.73 9.580
HR 2562 b 34.04 20.30 30.000 1.11 6471 F5 V 1.30 6.110 0.60
HR 8799 d 39.40 37 000.0 24.00 10.000 1.20 7400 A5 5.953 0.03
HD 156279 c 36.23 4191.0 8.600 (†) 0.23 281.0 5453 G6 0.95 8.100
GJ 649 b 10.38 598.3 1.14 0.328 (†) 0.30 172.0 3700 M0.5 0.54 9.690
GJ 504 b 17.54 43.50 4.000 6234 G0 V 1.22 5.220 0.16
HR 8799 c 39.40 69 000.0 38.00 10.000 1.20 7400 A5 5.953 0.03
47 UMa d 13.80 14 002.0 11.60 1.640 (†) 0.16 290.0 5892 G0 V 1.03 5.050 7.30
HR 8799 b 39.40 170 000.0 68.00 7.000 1.20 7400 A5 5.953 0.03
VHS J12-12 b (d) 12.70 102.00 11.200 2620 M7.5 0.07 17.759 0.23
2MASS J02-39 b (e) 39.40 156.00 13.900 1.44 3064 M6 0.11 0.04
HD 34445 g 46.15 5700.0 6.36 0.380 (†) 0.03 54.9 5879 G0 V 1.14 7.328
2MASS J01-24 b (f) 36.00 52.00 24.500 3530 M3.5 V 0.40 14.240 0.12
HN Peg b 18.13 773.00 21.999 1.05 5974 G0 IV-V 1.10 5.950 3.10
Ross 458 c 11.51 1168.00 6.285 1.22 3621 M0.5 0.49 9.720
HD 196067 b 39.98 3638.0 5.02 6.900 (†) 0.66 328.2 6017 G1 V 1.29 6.030 3.30
WD 0806-661 b 19.20 2500.00 7.500 0.62 1.50
GU Psc b 48.00 2000.00 11.300 1.26 M3 0.33 13.550 0.10
HD 142022 A b 34.31 1928.0 2.93 4.440 (†) 0.53 5421 K0 0.90 7.700
HD 133131 A c 47.00 3568.0 4.49 0.420 (†) 0.49 280.0 5799 G2 V 0.95 8.400 9.70

Notes. For reference, we list all planets accessible in the optimistic CGI scenario, including all possible values of Paccess and host-star magnitudes. The quoted values correspond mainly to the information in the NASA Exoplanet Archive as of September 16, 2020 (see Sect. 4). The parameters for bet Pic c were obtained from Nowak et al. (2020) because the quoted values in the NASA Archive show no upper or lower uncertainties. For DE CVn b, the inclination value was obtained from Han et al. (2018) and the corresponding uncertainties, from van den Besselaar et al. (2007). (†) Indicates that the Mp value corresponds to Mp sin(i). We note that, in those cases where the quoted uncertainties are 0.00, this is a result of insufficient significant figures in the rounding. We did not include upper or lower uncertainties for those cases in which they were not reported in the NASA Archive. In those cases where the quoted uncertainties of e reach nonphysical values (e.g. e < 0 for HD 154345 b, HD 114783, c or HD 62509 b), we truncate our sampling to a physical range of values. (a) 2MASS J21402931+1625183 A b, (b) WISEP J121756.91+162640.2 A b, (c)CFBDSIR J145829+101343 b, (d)VHS J125601.92-125723.9 b, (e)2MASS J02192210-3925225 b, (f)2MASS J01225093-2439505 b.

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