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Table F.1

Main characteristics of our targets, along with the source of data.

Name Spectral type Ref. m V [mag] Number of spectra

ALS/BD/HD Other AU C EL ESPa ESPR FE FI G HA HE M N S

U
Alb B&C

Slow rotators
HD 214680 10 Lac O9V 1 4.88 1
HD 46328 ξ1 CMa B0.5IV 2 4.33 1
HD 57682 O9.2IV 1 6.43 5
HD 149438 τ Sco B0V 3 2.81 2

Fast rotators
ALS 864 O9V 4 10.63 1
ALS 18675 ... 1 13.60 1
BD +60°594 O9V 3 9.30 1 1
BD +34°1058 O8nn 2 8.84 1
HD 13268 ON8.5IIIn 1 8.18 62 2 3
HD 14434 O5.5Vnn((f))p 1 8.49 6 8 1
HD 14442 O5n(f)p 1 9.27 38
HD 15137 O9.5II-IIIn 1 7.86 1 3
HD 15642 O9.5II-IIIn 1 8.55 3
HD 28446A 1 Cam A B0IIIn 2 5.77 14
HD 41161 O8Vn 1 6.76 1 3 22
HD 41997 O7.5Vn((f)) 5 8.46 1
HD 46056 O8Vn 1 8.16 8 1
HD 46485 O7V((f))nz 1 8.27 1 1
HD 52266 O9.5IIIn 1 7.23 6 2 1
HD 52533 O8.5IVn 1 7.68 1 2 2 1 1
HD 53755 V569 Mon B0.5V 6 6.49 1
HD 66811 ζ Pup O4I(n)fp 1 2.25 2
HD 69106 O9.7IIn 1 7.13 3 4 1
HD 74920 O7.5IVn((f)) 1 7.54 3 1
HD 84567 B0.5IIIn 7 6.45 2
HD 90087 O9.2III(n) 1 7.80 2
HD 92554 O9.5III 8 9.50 2
HD 93521 O9.5IIInn 1 7.03 20 2 1
HD 102415 ON9IV:nn 1 9.28 1 4
HD 117490 ON9.5IIInn 1 8.89 8
HD 124979 O7.5IV(n)((f)) 1 8.51 2
HD 149757 ζ Oph O9.2 IVnn 1 2.56 1 1 1
HD 150574 ON9III(n) 1 8.50 2
HD 163892 O9.5IV(n) 1 7.44 3 12 2
HD 172367 B0V 3 9.54 1
HD 175876 O6.5III(n)(f) 1 6.94 1 11
HD 184915 κ Aql B0.5III 3 4.96 4 3 1
HD 188439 V819 Cyg B0.5IIIpvar 3 6.28 4 5 1
HD 191423 ON9II-IIInn 1 8.03 7 2 2 2 1
HD 192281 V2011 Cyg O4.5V(n)((f)) 1 7.55 37 4 1
HD 198781 B0.5V 2 6.45 5
HD 203064 68 Cyg O7.5IIIn((f)) 1 5.00 1 3 4
HD 210839 λ Cep O6.5I(n)fp 1 5.05 1 6 1
HD 228841 O6.5Vn((f)) 1 9.01 1

Notes. The slow rotators are used for validation purposes (see Sect. 6). Magnitudes in the V band are from the SIMBAD database. For data sources, AU corresponds to AURELIE, C to CORALIE, EL to ELODIE, ESPa to ESPaDOnS, ESPR to ESPRESSO, FE to FEROS, FI to FIES, G to GOSSS (Alb to Albireo and B&C to Boller & Chivens), HA to HARPS, HE to HEROS, M to MIKE, N to NARVAL, S to SOPHIE, and U to UCLES.

Reference. For spectral types: [1] Sota et al. (2011, 2014); [2] Lesh (1968); [3] Morgan et al. (1955); [4] Fitzgerald & Moffat (1975); [5] Blaauw (1961); [6] Murphy (1969); [7] Hiltner et al. (1969); [8] Humphreys (1973).

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