Table A.1
Examples of SED fitting results
InternallD | RA (deg) | DEC (deg) | ndpt | Flux Code | Prob W3 | Prob W4 | Distance (pc) | Model Set | nfits | ![]() |
R* (R⊙ | T* (K) | L* (L⊙) | M* (M⊙) | Age (Myr) | Inclination (°) | Class | Stage |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
ID7166 | 83.57055 | -6.54707 | 13 | M1 | 0.03 | 363.62 | spubsmi | 1 | 238.95 | 0.62 | 3523 | 0.05 | 0.55 | 55.7 | 28.04 | Class II | Stage II | |
ID9189 | 85.06181 | -6.34854 | 10 | W4 | 1.00 | 1.00 | 368.06 | sp-s-i | 10 | 45.26 | 0.88 | 6044 | 0.93 | 1.05 | 36.1 | 27.56 | Class II | Stage II |
ID1738 | 79.22729 | -1.44311 | 6 | W3 | 0.99 | 311.13 | s—s-i | 21 | 39.5 | 1.61 | 5594 | 2.28 | 1.40 | 9.09 | 45.00 | Class III | Stage III | |
ID26196 | 85.12050 | 9.24075 | 6 | W3 | 0.56 | 400.01 | s—s-i | 11 | 23.5 | 1.11 | 4506 | 0.46 | 0.95 | 8.50 | 45.00 | Class III | Stage III | |
ID4996 | 83.18252 | -0.45422 | 9 | P3 | 0.98 | 1.00 | 326.71 | sp-hmi | 1 | 131 | 2.49 | 6661 | 11.01 | 1.70 | 7.89 | 5.01 | Class II | Stage II |
ID27106 | 86.91462 | 7.78719 | 6 | W3 | 0.67 | 400.01 | s—smi | 18 | 53.1 | 1.49 | 4844 | 1.10 | 1.25 | 5.35 | 45.00 | Class III | Stage III | |
ID18481 | 82.69350 | 8.78547 | 6 | W4 | 0.94 | 0.98 | 397.38 | s-u-smi | 30 | 9.57 | 1.48 | 4475 | 0.79 | 1.00 | 3.86 | 9.34 | Class II | Stage I |
ID4488 | 85.79479 | -8.56539 | 9 | Ml | 0.99 | 1.00 | 400.01 | s-u-hmi | 1 | 85.4 | 1.48 | 3922 | 0.47 | 0.70 | 2.82 | 78.28 | Class II | Stage I |
ID378 | 85.36927 | 9.17952 | 7 | W4 | 1.00 | 0.97 | 397.63 | sp-s-i | 24 | 39.26 | 1.27 | 3196 | 0.15 | 0.30 | 2.12 | 64.78 | Class II | Stage II |
ID5163 | 84.82848 | -2.51479 | 14 | P3 | 1.00 | 1.00 | 409.63 | sp-smi | 10 | 156 | 1.82 | 3947 | 0.72 | 0.65 | 1.42 | 35.00 | Class II | Stage II |
ID20380 | 87.78089 | 3.16753 | 8 | P3 | 0.94 | 409.79 | s-ubsmi | 27 | 65.2 | 2.11 | 4571 | 1.75 | 1.00 | 1.30 | 21.18 | Class III | Stage I | |
ID5098 | 84.51990 | -1.28853 | 7 | W4 | 0.99 | 1.00 | 346.54 | s-p-hmi | 1 | 23.9 | 1.52 | 3308 | 0.25 | 0.30 | 1.27 | 45.00 | Class II | Stage I |
ID 1434 | 87.02274 | 8.59186 | 7 | W4 | 1.00 | 1.00 | 393.90 | s-p-smi | 1 | 54.9 | 2.05 | 3439 | 0.53 | 0.30 | 0.70 | 45.00 | Class II | Stage I |
ID20379 | 87.46348 | 2.88613 | 7 | W4 | 1.00 | 0.95 | 411.25 | s-pbhmi | 1 | 65 | 2.11 | 3610 | 0.68 | 0.35 | 0.63 | 85.66 | Class II | Stage I |
ID7239 | 85.3521 | -8.94225 | 15 | Ml | 1.00 | 1.00 | 465.0 | sp-hmi | 1 | 182.3 | 2.65 | 3966 | 1.56 | 0.5 | 0.43 | 55.33 | Class II | Stage II |
ID3525 | 88.42046 | 1.63725 | 10 | P3 | 1.00 | 1.00 | 334.92 | spubsmi | 3 | 114 | 3.29 | 3887 | 2.23 | 0.45 | 0.18 | 30.93 | Class II | Stage II |
ID4777 | 84.69388 | -7.09372 | 17 | L | 0.81 | 0.96 | 400.01 | spubhmi | 1 | 681 | 2.46 | 3314 | 0.66 | 0.25 | 0.17 | 52.74 | Class II | Stage I |
ID1447 | 80.72661 | 4.94878 | 7 | W4 | 1.00 | 1.00 | 350.46 | s-ubhmi | 2 | 60.4 | 2.41 | 3151 | 0.51 | 0.16 | 0.08 | 41.26 | Class II | Stage I |
ID9858 | 86.18356 | -1.61107 | 10 | P3 | 1.00 | 1.00 | 477.28 | sp-h-i | 3 | 99.7 | 3.46 | 2969 | 0.84 | 0.14 | 0.01 | 14.00 | Class II | Stage II |
ID9045 | 86.90238 | 0.33506 | 7 | L | 1.00 | 0.98 | 400.01 | spu-hmi | 1 | 21.5 | 10.24 | 4034 | 25.02 | 0.65 | 0.01 | 9.30 | Class I | Stage I |
Notes. Example of 20 SED fitting results, sorted by age. The columns are as follows:(l) internal source identifier. (2) and (3) source coordinates in units of degrees. (4) number of data points used in the fit. (5) flux codes, which denotes the longest detected wavelength for each source (6) and (7) reliability probability of the WISE W3 and W4 detections. (8) distance based on GaiaDR3 parallax. Column (9) is the models used for fitting. (10) number of model fits attempted (11) (χ2)per data point for the best-fit model from the most likely model set. (12)–(17) list properties derived from the PARSEC models: radius, temperature, luminosity, mass. age. and inclination of the system. Column (18) corresponds to the class label, while column (19) lists the derived evolutionary stage. The distance 400.001 (average OSFC distance) was adopted in cases where the parallax measurement was either unavailable or unreliable.
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