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Table 3.

Intrinsic properties of stars with available spectroscopy.

Star Sp. type log Teff (GBP − GRP)0 AGRP MGRP
J183105.38−020424.8 A9 3.869 0.309 6.731 −1.002
J183114.83−020350.0 (1) B2 4.314 −0.348 5.215 −2.920
J183119.37−021229.5 B2 4.314 −0.348 4.596 −2.499
J183122.58−020531.6 (1) B5 4.196 −0.246 5.707 −1.711
J183123.96−020410.8 (1) B1 4.415 −0.425 5.958 −2.766
J183123.97−020529.5 (1) B8e 4.090 −0.156 5.997 −2.462
J183124.82−022008.4 B2 4.314 −0.348 4.425 −1.603
J183126.02−020517.0 (1) K:e 3.647 1.325 5.209 1.164
J183127.66−020509.7 (1) B2: 4.314 −0.348 7.079 −1.416
J183127.81−020521.8 (1) A0:e
J183127.83−020523.7 (1) O9.5 (2) 4.501 −0.487 6.350 −4.016
J183128.00−020517.2 (1) B7 4.146 −0.206 6.879 −0.766
J183129.61−020833.8 (1) B8 4.090 −0.156 6.693 −1.215
J183132.18−021531.2 G5 3.753 0.820 3.085 3.907
J183139.90−021842.9 A5 3.908 0.145 3.319 1.066
J183140.76−020931.3 A5 3.908 0.145 4.317 1.443
J183144.16−021618.2 K7 3.613 1.547 3.893 2.991
J183144.27−021621.2 M2: 3.551 2.290 3.667 4.763
J183149.20−021152.8 B5: 4.196 −0.246 5.016 −1.025
J183153.40−020959.9 K2 3.708 1.016 4.445 1.375
J183204.02−021353.4 B2 4.314 −0.348 5.624 −2.102

Notes. (1) Member of the central cluster. (2) Classification adopted from Shuping et al. (2012).

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