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Table D.1

Results of the spectroscopic analysis of the stars in the sample (extract).

ID 1 b SpCa υ sin ib υcmac Teff log𝑔d 1 ξ 1 YHe 1 log Q q Ref. file SNR
[deg] [deg] [km s−1] [km s−1] [K] [km s−1]
HD 164032 0.8767 −3.237 Bl/2Ib 108 50 23300800+700$23300_{ - 800}^{ + 700}$ 2.90.1+0.1$2.9_{ - 0.1}^{ + 0.1}$ = 18 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ < 14.00.0+0.3$ - 14.0_{ - 0.0}^{ + 0.3}$ 2 HD164032_20220830_201330_M_V85000_log 106
HD 164019 1.9099 −2.6166 09.5IVp 78 46 31000300+300$31000_{ - 300}^{ + 300}$ 3.30.1+0.0$3.3_{ - 0.1}^{ + 0.0}$ = 15 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ = 13.60.1+0.2$ - 13.6_{ - 0.1}^{ + 0.2}$ 1 HD164019_20080608_075144_F_V48000 183
HD 163613 2.0881 −1.9638 Β H/II 71 78 24400700+600$24400_{ - 700}^{ + 600}$ 2.90.1+0.1$2.9_{ - 0.1}^{ + 0.1}$ = 20 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ = 13.50.2+0.2$ - 13.5_{ - 0.2}^{ + 0.2}$ 1 HD163613_20200804_213522_N_V25000 96
HD 160430 3.7823 3.5878 Β 2II 20 46 22799500+500$22799_{ - 500}^{ + 500}$ 3.30.1+0.1$3.3_{ - 0.1}^{ + 0.1}$ = 13 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ < 13.90.1+0.1$ - 13.9_{ - 0.1}^{ + 0.1}$ 3 HD160430_20200802_220513_N_V25000 96
HD 164741 5.164 −1.6449 B1III(2) 20 32 250991200+1400$25099_{ - 1200}^{ + 1400}$ 3.60.2+0.2$3.6_{ - 0.2}^{ + 0.2}$ = 8 = 0.20.0+0.0$0.2_{ - 0.0}^{ + 0.0}$ < 14.00.0+0.4$ - 14.0_{ - 0.0}^{ + 0.4}$ 1 HD164741_20180731_223907_M_V85000 38
HD 173502 5.3641 −12.2722 B0.5III(2) 131 22 26600900+600$26600_{ - 900}^{ + 600}$ 3.60.1+0.1$3.6_{ - 0.1}^{ + 0.1}$ = 13 = 0.20.0+0.0$0.2_{ - 0.0}^{ + 0.0}$ < 14.00.0+0.3$ - 14.0_{ - 0.0}^{ + 0.3}$ 3 HD173502_20190710_003102_N_V25000 93
HD 156779 5.4256 10.3249 Β 211 97 39 18100900+600$18100_{ - 900}^{ + 600}$ 3.00.1+0.1$3.0_{ - 0.1}^{ + 0.1}$ = 13 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ < 14.00.0+0.4$ - 14.0_{ - 0.0}^{ + 0.4}$ 1 HD156779_20210621_224538_M_V85000_log 80
HD 168941 5.821 −6.3128 09.5IVp 107 91 30200300+400$30200_{ - 300}^{ + 400}$ 3.20.0+0.0$3.2_{ - 0.0}^{ + 0.0}$ = 16 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ < 14.00.0+0.2$ - 14.0_{ - 0.0}^{ + 0.2}$ 1 HD168941_20060512_083253_F_V48000 363
HD 165016 5.8521 −1.5791 B0V(2) 19 21 30299300+500$30299_{ - 300}^{ + 500}$ 3.90.1+0.1$3.9_{ - 0.1}^{ + 0.1}$ = 6 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ > 13.00.2+0.1$ - 13.0_{ - 0.2}^{ + 0.1}$ 1 HD165016_20200803_211628_N_V25000 109
HD 168750 6.1891 −5.8526 Β IIb 33 50 25600700+600$25600_{ - 700}^{ + 600}$ 3.30.1+0.1$3.3_{ - 0.1}^{ + 0.1}$ = 13 = 0.20.0+0.1$0.2_{ - 0.0}^{ + 0.1}$ < 13.90.1+0.3$ - 13.9_{ - 0.1}^{ + 0.3}$ 1 HD168750_20220826_215128_M_V85000_log 84
HD 149757 6.2812 23.5877 09.2IVnn 410 0 30700600+600$30700_{ - 600}^{ + 600}$ 3.30.1+0.1$3.3_{ - 0.1}^{ + 0.1}$ = 16 = 0.20.0+0.0$0.2_{ - 0.0}^{ + 0.0}$ = 13.00.6+0.1$ - 13.0_{ - 0.6}^{ + 0.1}$ 1 HD149757_20210622_234421_M_V85000_log 435
HD 164018 6.6528 0.1591 Bl/2Ib 142 38 29400800+600$29400_{ - 800}^{ + 600}$ 3.60.1+0.1$3.6_{ - 0.1}^{ + 0.1}$ = 15 = 0.10.0+0.1$0.1_{ - 0.0}^{ + 0.1}$ < 14.00.0+0.4$ - 14.0_{ - 0.0}^{ + 0.4}$ 1 HD164018_20180920_215654_N_V25000 70
HD 165132 6.7522 −1.2103 09.7V(2) 127 20 32500700+1100$32500_{ - 700}^{ + 1100}$ 4.00.1+0.2$4.0_{ - 0.1}^{ + 0.2}$ = 12 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ < 14.00.0+0.4$ - 14.0_{ - 0.0}^{ + 0.4}$ 1 HD165132_20190709_222717_N_V67000 73
HD 164971 6.8868 −0.9279 BOIa 43 76 27500700+800$27500_{ - 700}^{ + 800}$ 3.10.1+0.2$3.1_{ - 0.1}^{ + 0.2}$ = 16 = 0.10.0+0.1$0.1_{ - 0.0}^{ + 0.1}$ < 13.60.4+0.2$ - 13.6_{ - 0.4}^{ + 0.2}$ 1 HD164971_20110902_222249_M_V85000 60
HD 163892 7.1516 0.6161 09.5IV(n) 216 0 31600500+600$31600_{ - 500}^{ + 600}$ 3.50.1+0.1$3.5_{ - 0.1}^{ + 0.1}$ = 12 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ < 13.90.1+0.2$ - 13.9_{ - 0.1}^{ + 0.2}$ 1 HD163892_20210623_001114_M_V85000_log 142
HD 164402 7.1621 −0.0339 B01b(3) 54 86 28900400+300$28900_{ - 400}^{ + 300}$ 3.20.1+0.1$3.2_{ - 0.1}^{ + 0.1}$ = 18 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ = 13.60.1+0.1$ - 13.6_{ - 0.1}^{ + 0.1}$ 1 HD164402_20220829_203450_M_V85000_log 144
HD 164637 7.3435 −0.2284 B0Ib/II 35 72 29200200+200$29200_{ - 200}^{ + 200}$ 3.30.0+0.0$3.3_{ - 0.0}^{ + 0.0}$ = 15 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ < 13.90.1+0.2$ - 13.9_{ - 0.1}^{ + 0.2}$ 1 HD164637_20130821_042119_F_V48000 327
HD 164359 7.6967 0.338 BUI 77 35 30099400+500$30099_{ - 400}^{ + 500}$ 3.90.1+0.1$3.9_{ - 0.1}^{ + 0.1}$ = 9 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ < 14.00.0+0.3$ - 14.0_{ - 0.0}^{ + 0.3}$ 2 HD164359_20220830_210910_M_V85000_log 131
HD 158661 8.2908 9.0476 Β0ΙΙ 60 96 26900500+400$26900_{ - 500}^{ + 400}$ 3.90.1+0.1$3.9_{ - 0.1}^{ + 0.1}$ = 22 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ = 13.30.1+0.2$ - 13.3_{ - 0.1}^{ + 0.2}$ 1 HD158661_20210623_010823_M_V85000_log 151
HD 165812 8.476 −1.1091 B1/2II 42 34 25099700+700$25099_{ - 700}^{ + 700}$ 3.70.1+0.1$3.7_{ - 0.1}^{ + 0.1}$ = 8 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ < 13.90.1+0.2$ - 13.9_{ - 0.1}^{ + 0.2}$ 1 HD165812_20200803_215831_N_V25000 113
HD 166852 8.5074 −2.3235 B01a/ab 45 130 320001200+1400$32000_{ - 1200}^{ + 1400}$ 3.40.2+0.2$3.4_{ - 0.2}^{ + 0.2}$ = 16 = 0.10.0+0.1$0.1_{ - 0.0}^{ + 0.1}$ < 14.00.0+0.5$ - 14.0_{ - 0.0}^{ + 0.5}$ 1 HD166852_20190709_220222_N_V67000 46
HD 159864 8.5231 7.3825 Β IIb 88 98 27300400+600$27300_{ - 400}^{ + 600}$ 3.10.1+0.1$3.1_{ - 0.1}^{ + 0.1}$ = 18 = 0.10.0+0.1$0.1_{ - 0.0}^{ + 0.0}$ < 13.70.3+0.2$ - 13.7_{ - 0.3}^{ + 0.2}$ 1 HD159864_20200502_050638_N_V25000 110
HD 165516 8.9268 −0.4446 Bl/2Ib 47 67 25900400+300$25900_{ - 400}^{ + 300}$ 3.10.1+0.1$3.1_{ - 0.1}^{ + 0.1}$ = 17 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ = 13.70.2+0.2$ - 13.7_{ - 0.2}^{ + 0.2}$ 1 HD165516_20200803_212544_N_V46000 144
HD 165892 9.1729 −0.8113 Β 211 74 42 21600900+1000$21600_{ - 900}^{ + 1000}$ 3.40.2+0.1$3.4_{ - 0.2}^{ + 0.1}$ = 11 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ < 14.00.0+0.3$ - 14.0_{ - 0.0}^{ + 0.3}$ 1 HD165892_20130412_050607_M_V85000 62
HD 149363 9.8524 26.6906 Bl/2Ib 88 62 27300200+400$27300_{ - 200}^{ + 400}$ 3.30.1+0.1$3.3_{ - 0.1}^{ + 0.1}$ = 16 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ < 14.00.0+0.3$ - 14.0_{ - 0.0}^{ + 0.3}$ 1 HD149363_20190707_211718_N_V25000 194
HD 164438 10.3529 1.7886 09.2IV 61 105 31300400+400$31300_{ - 400}^{ + 400}$ 3.30.0+0.0$3.3_{ - 0.0}^{ + 0.0}$ = 13 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ < 14.00.0+0.5$ - 14.0_{ - 0.0}^{ + 0.5}$ 1 HD164438_20080514_092403_F_V48000 303
HD 166546 10.358 -0.9242 09.5IV 31 73 31000200+400$31000_{ - 200}^{ + 400}$ 3.40.0+0.0$3.4_{ - 0.0}^{ + 0.0}$ = 12 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ < 14.00.0+0.1$ - 14.0_{ - 0.0}^{ + 0.1}$ 1 HD166546_20080609_082259_F_V48000 284
HD 167264 10.4557 −1.7408 09.7Iab 80 67 28200300+300$28200_{ - 300}^{ + 300}$ 3.10.0+0.0$3.1_{ - 0.0}^{ + 0.0}$ = 22 = 0.10.0+0.0$0.1_{ - 0.0}^{ + 0.0}$ = 13.20.0+0.0$ - 13.2_{ - 0.0}^{ + 0.0}$ 1 HD167264_20100907_202837_N_V46000 273

Notes. (a)We adopted the recommended spectral classification quoted in the SIMBAD astronomical database (Wenger et al. 2000) except for the cases indicated with an upper index and the following: (1) de Burgos et al. (2020); (2) de Burgos et al. (2023); (3) Negueruela et al. (2024). For HD 168021, HD 168183, and HD187879, the SIMBAD classification included a second component, but we have only included the first. In the case of the O-type stars, most of the classifications are adopted from the GOSSS series of papers (Sota et al. 2011, 2014; Maíz Apellániz et al. 2016). (b)We adopt a global uncertainty for υ sin ì of 15 km s−1 based on the average value. (c)We adopt a global uncertainty for υmíc of 20 km s−1 based on the average value. Based on the results by Simón-Díaz & Herrero (2014), we assigned = 0 km s−1 to those cases in which υ sin i > 180 km s−1. (d)The values of log 𝑔 have not been corrected for centrifugal acceleration. The full table is available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/.

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