Table D.1.
PMS candidates (p ≥ 50%, 8470 sources) ordered by probability.
| Gaia source id | RA | Dec | Probability | Probability | Probability | Vhtg | Gvar | ||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| h:m:s | deg:m:s | PMS | CBe | Other | |||||||
| 189190423171051136 | 05:39:18.1 | +36:17:16 | 1.00±0.00 | (7.8 ± 2.0)×10−6 | (4.2 ± 1.6)×10−6 | −52.13 | 158.74 | ||||
| 513068993519575808 | 01:39:32.5 | +64:53:02 | 1.00±0.00 | (4.18 ± 0.91)×10−5 | (7.7 ± 2.9)×10−6 | −66.16 | 165.17 | ||||
| 5546522453993928960 | 08:12:40.5 | −34:14:12 | 1.00±0.00 | (4.4 ± 2.0)×10−5 | (1.38 ± 0.58)×10−5 | −117.08 | 225.56 | ||||
| 181175743617347328 | 05:23:04.3 | +33:28:46 | 1.00±0.00 | (1.67 ± 0.44)×10−4 | (4.7 ± 2.0)×10−6 | −47.67 | 131.31 | ||||
| 3430718965791698176 | 05:52:51.7 | +26:47:30 | 1.00±0.00 | (3.04 ± 0.96)×10−4 | (3.6 ± 1.0)×10−5 | –67.90 | 152.91 | ||||
| 3046391307734381184 | 07:09:22.3 | −10:30:57 | 1.00±0.00 | (2.06 ± 0.55)×10−4 | (1.52 ± 0.57)×10−4 | −44.33 | 77.08 | ||||
| 3449189833426211840 | 05:32:13.9 | +34:06:01 | 1.00±0.00 | (8.0 ± 2.8)×10−5 | (2.8 ± 1.8)×10−4 | −107.39 | 183.40 | ||||
| 189577661722195840 | 05:37:53.2 | +37:24:56 | 1.00±0.00 | (2.61 ± 0.60)×10−4 | (1.52 ± 0.51)×10−4 | −66.15 | 117.40 | ||||
| 2006046771487587328 | 22:24:13.8 | +56:11:33 | 1.00±0.00 | (2.3 ± 1.1)×10−4 | (2.38 ± 0.99)×10−4 | −117.72 | 162.47 | ||||
| 4279295067717293696 | 18:47:32.6 | +02:12:06 | 1.00±0.00 | (1.31 ± 0.21)×10−4 | (3.82 ± 0.94)×10−4 | –33.04 | 96.61 | ||||
| 3114712967419900544 | 07:09:42.8 | +01:53:11 | 1.00±0.00 | (5.5 ± 2.4)×10−5 | (5.4 ± 4.0)×10−4 | −46.52 | 143.75 | ||||
| 3102576519414606464 | 06:58:34.4 | −03:56:46 | 1.00±0.00 | (1.75 ± 0.58)×10−4 | (4.3 ± 1.2)×10−4 | −26.55 | 58.08 | ||||
| ... | ... | ... | ... | ... | ... | ... | ... | ||||
| GBP | G | GRP | IPHAS or VPHAS+ | r | i | Hα | AllWISE | J | H | Ks | |
| (mag) | (mag) | (mag) | name | (mag) | (mag) | (mag) | name | (mag) | (mag) | (mag) | |
| 15.97 | 15.04 | 14.04 | J053918.09+361716.2 | 13.78 | 13.06 | 13.21 | J053918.08+361716.1 | 12.98 | 11.23 | 9.79 | |
| 14.34 | 13.80 | 12.98 | J013932.55+645302.3 | 12.91 | 12.43 | 12.35 | J013932.53+645302.2 | 11.43 | 10.21 | 9.11 | |
| 14.97 | 14.18 | 13.20 | J081240.5–341411.7 | 12.86 | 12.19 | 11.99 | J081240.50–341411.7 | 10.86 | 10.08 | 9.59 | |
| 14.89 | 14.40 | 13.66 | J052304.26+332846.5 | 13.80 | 13.24 | 12.90 | J052304.26+332846.4 | 12.01 | 11.12 | 10.25 | |
| 14.40 | 13.94 | 13.05 | J055251.75+264730.2 | 12.62 | 12.22 | 12.28 | J055251.74+264730.0 | 12.16 | 11.04 | 10.06 | |
| 16.75 | 15.56 | 14.31 | J070922.3–103057.0 | 16.04 | 14.94 | 14.78 | J070922.28–103057.0 | 12.47 | 10.98 | 9.90 | |
| 16.17 | 14.76 | 13.63 | J053213.92+340601.5 | 13.70 | 12.39 | 13.25 | J053213.92+340601.4 | 10.80 | 9.83 | 8.83 | |
| 14.73 | 13.68 | 12.63 | J053753.15+372456.1 | 14.30 | 13.07 | 13.80 | J053753.15+372456.0 | 10.54 | 9.83 | 9.31 | |
| 14.00 | 13.31 | 12.40 | J222413.78+561133.2 | 13.63 | 12.92 | 13.29 | J222413.75+561133.2 | 9.56 | 8.69 | 8.01 | |
| 15.15 | 14.11 | 13.05 | J184732.62+021205.9 | 15.01 | 13.84 | 14.23 | J184732.61+021205.7 | 11.34 | 9.97 | 8.79 | |
| 13.62 | 11.79 | 10.19 | J070942.85+015311.0 | 13.86 | 11.84 | 13.15 | J070942.75+015311.1 | 8.20 | 6.62 | 5.25 | |
| 18.24 | 17.57 | 16.41 | J065834.4–035645.6 | 21.41 | 20.84 | 20.13 | J065834.39–035645.6 | 13.73 | 12.40 | 11.38 | |
| ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | |
| W1 | W2 | W3 | W4 | RUWE | Parallax (ϖ) | Distance |  |
MG | GBP − GRP | HAeBe | Flag |
| (mag) | (mag) | (mag) | (mag) | [mas] | [pc] | (mag) | (mag) | (mag) | |||
| 7.90 | 7.05 | 4.84 | 3.23 | 1.36 | 0.636 ± 0.048 |
 |
1.06 | 3.09 | 1.41 | Yes | Var |
| 7.95 | 7.26 | 5.41 | 3.90 | 1.86 | 1.116 ± 0.029 |
 |
– | – | – | – | Var |
| 8.63 | 7.81 | 5.37 | 3.32 | 1.33 | 2.877 ± 0.025 |
 |
0.06 | 6.43 | 1.75 | – | Var, W3W4 |
| 9.12 | 8.39 | 6.35 | 4.21 | 1.37 | 0.234 ± 0.040 |
 |
1.04 | 0.51 | 0.72 | – | Var, W3W4 |
| 9.26 | 8.76 | 7.23 | 5.56 | 1.09 | 1.950 ± 0.032 |
 |
0.27 | 5.15 | 1.22 | Yes | Var |
| 7.19 | 5.90 | 3.19 | 1.06 | 3.28 | 1.00 ± 0.20 |
 |
– | – | – | – | Var, W3W4 |
| 6.92 | 5.79 | 3.95 | 2.94 | 1.01 | −0.068 ± 0.080 |
 |
– | – | – | – | GUMAP, Var |
| 8.34 | 7.37 | 5.01 | 3.66 | 1.32 | 0.025 ± 0.041 |
 |
– | – | – | – | Var, W3W4 |
| 7.06 | 5.99 | 3.79 | 2.43 | 1.72 | 0.326 ± 0.027 |
 |
– | – | – | – | Var, W3W4 |
| 7.61 | 6.97 | 4.84 | 3.10 | 1.30 | 1.614 ± 0.046 |
 |
1.99 | 3.19 | 1.13 | Yes | Var |
| 3.99 | 1.79 | 1.93 | 1.44 | 1.01 | 0.103 ± 0.089 |
 |
– | – | – | – | GUMAP, Var, W3W4 |
| 10.58 | 9.25 | 6.40 | 4.02 | 1.15 | 0.36 ± 0.11 |
 |
– | – | – | – | Var, W3W4 |
| ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... |
Notes. In boldface sources that are strong Herbig Ae/Be candidates according to their position on the HR diagram (MG < 6, 1361, see Fig. 5). These Herbig Ae/Be candidates are also indicated in the column “HAeBe”. This table is available in its entirety at the CDS with uncertainties of the magnitudes, quality flags, and rest of Gaia parameters together with angular distances from AllWISE and IPHAS or VPHAS+ sources to Gaia sources. A portion is shown here for guidance regarding its form and content. The probabilities are expressed to the precision of their uncertainties. Distances from Bailer-Jones et al. (2018). 
only traces the interstellar extinction. It is used to correct MG and GBP − GRP. 
, MG, and GBP − GRP are only presented for sources with RUWE< 1.4 and ϖ/σ(ϖ) ≥ 5. By construction Herbig Ae/Be candidates are astrometrically well behaved (RUWE< 1.4 and ϖ/σ(ϖ) ≥ 10). These constraints can be relaxed to obtain more Herbig Ae/Be candidates. The probabilities of the three categories sum up to 1. The different catalogue warning flags are discussed throughout the text and summarised in Appendix D.
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