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Table 1.

Target list.

Source Spectral V-band Type Pspin Porb e Distance (kpc) vsini References
name type (mag) var. (s) (days) Gaia EDR3 (‡) (km s−1)
IGR J00370+6122 BN0.7Ib 9.6 s 346 15.66 0.5 3.4 ± 0.2 135 ± 7 [1a], [1b]
2S 0114+65 B1Ia 11.0 s 9720 11.6 0.18 96 ± 20 [2a], [2b]
4U 0115+63 B0.2Ve 15.4 g 3.6 24.3 0.34 300 ± 50 [3a], [3b]
IGR J01363+6610 B1IV-Ve 13.3 g 5.8 ± 0.4 160 ± 20 [4a], [4b], [4c]
RX J0146.9+6121 (†) B1Ve 11.3 1400 303? 200 ± 30 [5a], [5b]
RX J0240.4+6112 B0Ve 10.8 g 26.5 0.54 2.5 ± 0.7 350 ± 8 [6a], [6b]
SWIFT J0243.6+6124 O9.5Ve 12.8 g 9.9 27.6 0.10 5.2 ± 0.3 210 ± 20 [7a], [7b]
V 0332+53 O8–9Ve 15.4 g,h 4.4 33.8 0.37 150 ± 30 [8a], [8b]
X Per B0Ve 6.1 g,h 838 250 0.11 215 ± 10 [9a], [9b]
RX J0440.9+4431 B0.2Ve 10.7 g,h 202.5 150 235 ± 15 [10a], [10b]
1A 0535+262 O9.7IIIe 9.2 g,h 105 111 0.47 225 ± 10 [11a], [11b]
IGR J06074+2205 B0.5Ve 12.2 i,h 373.2 6.0 ± 0.6 260 ± 20 [12]
MXB 0656–072 O9.5Ve 12.3 i 160.4 5101.2 0.4? 5.7 ± 0.5 [13a], [13b]
RX J0812.4–3114 B0.2IVe 12.7 g,h 31.9 80 240 ± 20 [14a], [14b]
Vela X–1 B0.5Ib 6.9 s 283 8.96 0.09 2.00 ± 0.06 116 ± 6 [15]
GRO J1008-57 B1Ve 15.3 g,h 93.5 249.5 0.68 3.54 ± 0.15 [16a], [16b]
RX J1037.5–5647 B0III-Ve 11.5 s 860 [17a], [17b]
1A 1118–616 O9.5IV-Ve 12.1 g,h 406.5 24 < 0.1 270 ± 25 [18a], [18b]
4U 1145–61 B0.2IIIe 9.0 g,h 292 186.5 > 0.5 280 ± 30 [19a], [19b]
GX 304–1 B0.7Ve 14.4 i,h 272 132.5 0.46 1.90 ± 0.05 330 ± 50 [20a], [20b]
KS 1947+300 B0Ve 14.5 s 18.7 40.4 0.03 310 ± 40 [21a], [21b]
Swift J2000.6+3210 (†) B0-2Ve 16.2 890 [22]
GRO J2058+42 O9.5-B0IV-Ve 14.9 i,h 192 110 250 ± 50 [23a], [23b]
SAX J2103.5+4545 (†) B0Ve 13.9 358 12.7 0.40 240 ± 20 [24a], [24b]
IGR J21343+4738 (†) B1IVe 14.1 320 365 ± 15 [25]
Cep X–4 (†) B1-2Ve 14.3 66.3 24.8? 460 ± 50 [26]
4U 2206+54 O9.5Ve 9.8 s,h 5550 19.2 0.15 315 ± 70 [27a], [27b], [27c]
SAX J2239.3+6116 B0Ve 14.4 g,h 1247 263 195 ± 20 [28]
MWC 656 B1.5IIIe 8.7 g 60.4 0.10 2.0 ± 0.1 313 ± 3 [29]

Notes. The fourth column indicates the type of variability of the periodograms as defined in Sect. 4.1 : g: frequency groups, i: isolated frequencies, s: stochastic variability, and h: high-frequency signals (applicable to TESS data only). (†)Ground-based data only; (‡)Bailer-Jones et al. (2021). Gaia distances are model dependent and may differ substantially in the various Data Releases (DR). Here we quote the distance obtained from EDR3 using https://dc.zah.uni-heidelberg.de/gedr3dist/q/cone/form. See also Arnason et al. (2021).

References. [1a] González-Galán et al. (2014); [1b] Grunhut et al. (2014); [2a] Crampton et al. (1985); [2b] Reig et al. (1996); [3a] Negueruela & Okazaki (2001); [3b] Raichur & Paul (2010); [4a] Reig et al. (2005b); [4b] Tomsick et al. (2011); [4c] vsini (Reig, priv. comm.); [5a] Reig et al. (1997b); [5b] Sarty et al. (2009); [6a] Aragona et al. (2009); [6b] Zamanov et al. (2013); [7a] Wilson-Hodge et al. (2018); [7b] (Reig et al. 2020); [8a] Negueruela et al. (1999); [8b] Doroshenko et al. (2016); [9a] Lyubimkov et al. (1997); [9b] Delgado-Martí et al. (2001); [10a] Reig et al. (2005a), [10b] Ferrigno et al. (2013); [11a] Haigh et al. (2004); [11b] Grundstrom et al. (2007a); [12] Reig et al. (2010b); [13a] Yan et al. (2012); [13b] Nespoli et al. (2012); [14a] Reig et al. (2001); [14b] Corbet & Peele (2000); [15] van Kerkwijk et al. (1995); [16a] Kühnel et al. (2013); [16b] Coe et al. (2007); [17a] Reig & Roche (1999a); [17b] Motch et al. (1997); [18a] Motch et al. (1988); [18b] Staubert et al. (2011); [19a] Janot Pacheco et al. (1982); [19b] Alfonso-Garzón et al. (2017); [20a] Parkes et al. (1980); [20b] Malacaria et al. (2017); [21a] Galloway et al. (2004); [21b] vsini (Reig, priv. comm.); [22] Masetti et al. (2008); [23a] (Wilson et al. 1998); [23b] (Kızıloğlu et al. 2007b); [24a] Baykal et al. (2000); [24b] Reig et al. (2004); [25] Reig & Zezas (2014a); [26] Bonnet-Bidaud & Mouchet (1998); [27a] Corbet et al. (2007); [27b] Blay et al. (2006); [27c] Reig et al. (2009); [28] Reig et al. (2017); [29] Zamanov et al. (2021).

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