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Table A.3

Astrometric and evolutionary parameters for the 29 unconfirmed post-AGB candidates.

Num Distance (pc) Low Dist. (pc) High Dist. (pc) AV T(eff) (K) Flag (T) Lo𝑔[L] Lo𝑔[L]min SED Flag
6 4007 3509 4603 0.09 3500 T1 3.19 3.05 3.33 stellar H
8 7877 7285 8653 < 0.01 7250 T2 2.92 2.83 3.01 stellar H
16 7633 6920 8251 1.40 11000 T3(1) 3.12 3.03 3.20 stellar H
23 2569 2382 2815 0.20 11750 T2 2.46 2.38 2.54 stellar H
32 2138 2058 2229 0.70 9500 T3(2) 3.16 3.12 3.19 stellar H
44 2568 2429 2706 0.30 7500 T3(3) 2.99 2.94 3.04 stellar H
46 4893 4514 5338 0.60 6750 T3(4) 3.19 3.11 3.27 stellar H
48 1446 1391 1510 0.85 22000 T3(5) 2.56 2.52 2.60 stellar -
57 945 921 964 0.40 6500 T3(6) 2.84 2.82 2.86 disc -
61 937 926 947 1.00 5750 T3(7) 2.06 2.05 2.07 shell -
66 1982 1915 2056 0.66 3750 T3(8) 2.37 2.33 2.40 shell -
69 1952 1895 2002 0.69 3750 T1 2.63 2.60 2.65 shell -
73 5266 4836 5721 4.00 1000 T3(8) 3.07 2.99 3.15 shell -
80 3226 3025 3469 5.55 6000 T1 2.76 2.70 2.83 shell -
81 2504 2408 2629 3.28 6750 T1 2.45 2.41 2.49 shell -
83 1978 1856 2105 2.50 4000 T3(9) 3.01 2.95 3.06 disc -
86 4277 3572 5089 5.80 8750 T3(8) 3.00 2.81 3.19 shell -
87 5204 4054 6718 2.00 3500 T3(8) 1.96 1.64 2.27 shell -
88 2533 2306 2812 4.53 3750 T1 2.94 2.84 3.04 shell -
90 4882 4170 5705 3.00 4250 T3(8) 2.27 2.10 2.43 shell -
91 5991 5520 6694 1.76 8250 T1 3.01 2.91 3.11 shell -
100 4898 4294 5685 4.79 5750 T1 3.01 2.87 3.16 disc -
101 6087 5536 6736 0.67 3500 T3(8) 3.15 3.06 3.25 shell -
105 1694 1631 1768 5.34 4250 T1 2.50 2.46 2.53 disc -
110 5710 4998 6635 < 0.01 14000 T3(10) 2.79 2.64 2.94 stellar H
130 1365 1313 1420 0.90 4750 T2 3.21 3.16 3.27 shell -
149 6299 5704 7065 0.47 4000 T3(9) 3.06 2.95 3.16 stellar H
154 4714 4378 5080 0.38 4000 T1 3.29 3.22 3.36 stellar -
155 2123 1943 2310 0.49 3500 T1 2.88 2.80 2.96 stellar -

Notes. (H): Suspected Halo star.

References. Temperatures are: (T1) obtained from SED fitting with AV from Stassun (2019), (T2): derived from Simbad spectral types, (T3): obtained from the literature (mainly for spectroscopic measurements): (1): Mooney et al. (2004), (2): Venn et al. (1998), (3): Kamath et al. (2022), (4): Gonzalez & Wallerstein (1992), (5): Hunger & Kaufmann (1973), (6): Kluska et al. (2022), (7): Ting et al. (2019), (8): Suárez et al. (2006), (9): Steinmetz et al. (2020), (10): Quin & Lamers (1992).

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