Table 1.
List of the 44 selected NS-HMXB sources and their Gaia EDR3 counterparts.
| Name | Type | Sp. type | Ref. | M [M⊙] | Ref. | Porb [d] | Ref. | Ecc. | Ref. | Gaia EDR3 source id. |
|---|---|---|---|---|---|---|---|---|---|---|
| IGR J00370+6122(a) | Be | B0.5II-III | [1] | 22.0 | [2] | 15.7 | [3] | 0.5 | [2] | 427234969757165952 |
| 1A 0114+650(b) | sg | B1Iae | [4] | 16.0 ± 2.0 | [5] | 11.6 | [6] | 0.2 | [7] | 524924310153249920 |
| 4U 0115+634(c) | Be | B0.2Ve | [8] | 17.5 | [9] | 24.3 | [10] | 0.3 | [10] | 524677469790488960 |
| IGR J01363+6610 | Be | B1Ve | [1] | 12.5 | [9] | 159.0 | [11] | – | – | 519352324516039680 |
| IGR J01583+6713(d) | Be | B2IVe+ | [12] | 12.5 | [9] | – | – | – | – | 518990967445248256 |
| LS I+61 303(e) | Be | B0Ve | [13] | 12.5 | [14] | 26.5 | [15] | 0.5 | [16] | 465645515129855872 |
| EXO 0331+530(c) | Oe | O8.5Ve | [17] | 18.8 | [18] | 36.5 | [10] | 0.4 | [10] | 444752973131169664 |
| X Per(c) | Be | O9.5III | [19] | 15.5 | [20] | 250.3 | [21] | 0.1 | [21] | 168450545792009600 |
| XTE J0421+560 | sg | B0/2I[e]:sgB[e] | [22] | – | – | – | – | – | – | 276644757710014976 |
| RX J0440.9+4431(d) | Be | B0.2Ve | [23] | 17.5 | [9] | 150.0 | [24] | – | – | 252878401557369088 |
| EXO 051910+3737.7 | Be | B0III-IVe | [25] | 17.5 | [9] | – | – | – | – | 184497471323752064 |
| 1A 0535+262(c) | Oe | O9.5III-Ve | [26] | 20.0 | [27] | 110.3 | [27] | 0.5 | [28] | 3441207615229815040 |
| HD 259440 | Be | B0pe | [29] | 15.7 ± 2.5 | [30] | 308.0 | [31] | 0.6 | [31] | 3131822364779745536 |
| SAX J0635.2+0533(f) | Be | B2V-B1IIIe | [32] | 9.6 | [9] | 11.2 | [33] | 0.3 | [33] | 3131755947406031104 |
| IGR J08262−3736 | Be | OBV | [34] | – | – | – | – | – | – | 5541793213959987968 |
| IGR J08408−4503 | sg | O8.5Ib-II(f)p | [35] | 33.0 | [36] | 9.5 | [36] | 0.6 | [36] | 5522306019626566528 |
| Vela X-1(c) | sg | B0.5Iae-1b | [37] | 26.0 ± 1.0 | [38] | 9.0 | [39] | 0.1 | [39] | 5620657678322625920 |
| GRO J1008−57(d) | Be | B0e | [40] | 17.5 | [9] | 249.5 | [41] | 0.7 | [41] | 5258414192353423360 |
| 2FGL J1019.0−5856 | Oe | O6V | [42] | 23.0 ± 3.0 | [43] | 16.5 | [44] | 0.3 | [44] | 5255509901121774976 |
| 1A 1118−615(d) | Oe | O9.5III-Ve | [45] | 18.0 | [18] | 24.0 | [46] | – | – | 5336957010898124160 |
| 1E 1145.1−6141(d) | sg | B2Iae | [47] | 14.0 ± 4.0 | [48] | 14.4 | [49] | 0.2 | [49] | 5334851450481641088 |
| 2E 1145.5−6155 | Be | B1III-Ve | [50] | 12.5 | [9] | 187.5 | [41] | 0.5 | [41] | 5334823859608495104 |
| EXMS B1210−645 | Be | B2V | [51] | 9.6 | [9] | 6.7 | [46] | – | – | 6053076566300433920 |
| GX 301−2(c) | sg | B1.5Iaeq | [52] | 43.0 ± 10.0 | [53] | 41.5 | [53] | 0.5 | [53] | 6054569565614460800 |
| GX 304−1(c) | Be | B2Vne | [54] | 9.6 | [9] | 132.5 | [46] | – | – | 5863533199843070208 |
| PSR B1259−63(d) | Oe | O9.5Ve | [55] | 22.5 ± 7.5 | [56] | 1236.7 | [56] | 0.9 | [56] | 5862299960127967488 |
| IGR J14331−6112 | Be | BV-IIIe | [57] | – | – | – | – | – | – | 5878377736381364608 |
| 4U 1538−522(g) | sg | B0.2Ia | [58] | 20.0 | [59] | 3.7 | [59] | 0.1 | [59] | 5886085557746480000 |
| 1H 1555−552 | Be | B2IIIn | [60] | 9.6 | [9] | – | – | – | – | 5884544931471259136 |
| IGR J16195−4945 | Oe | ON9.7Iab | [61] | 27.8 | [18] | 16.0 | [46] | – | – | 5935509395659726592 |
| IGR J16465−4507(d) | sg | O9.5Ia | [62] | 27.8 | [18] | 30.2 | [41] | – | – | 5943246345430928512 |
| 4U 1700−377(c) | sg | O6Iafcp | [35] | 46.0 ± 5.0 | [38] | 3.4 | [63] | 0.0 | [63] | 5976382915813535232 |
| RX J1744.7−2713 | Be | B0.5V-IIIe | [64] | 14.6 | [9] | – | – | – | – | 4060784345959549184 |
| IGR J17544−2619(c) | sg | O9Ib | [65] | 23.0 ± 2.0 | [66] | 12.2 | [67] | 0.4 | [67] | 4063908810076415872 |
| LS 5039 | Oe | ON6.5V(f) | [68] | 23.0 | [69] | 3.9 | [70] | 0.3 | [70] | 4104196427943626624 |
| XTE J1855−026(d) | sg | B0Iaep | [71] | – | – | 6.0 | [71] | – | – | 4255891924062617088 |
| IGR J20006+3210(h) | Be | BV-III | [57] | – | – | – | – | – | – | 2033989790047905024 |
| RX J2030.5+4751 | Be | BVe | [72] | – | – | 46.0 | [41] | 0.4 | [41] | 2083644392294059520 |
| GRO J2058+42(i) | Be | O9.5-B0IV-Ve | [1] | 18.0 | [73] | 55.0 | [74] | – | – | 2065653598916388352 |
| SAX J2103.5+4545(c) | Be | B0Ve | [75] | 17.5 | [9] | 12.7 | [76] | 0.4 | [76] | 2162805896614571904 |
| IGR J21347+4737 | Be | B3V | [51] | 7.7 | [9] | – | – | – | – | 1978365123143522176 |
| Cep X-4(c) | Be | B1.5Ve:B1-B2Ve | [77] | 10.8 | [9] | 20.9 | [78] | – | – | 2178178409188167296 |
| 4U 2206+543(d) | Oe | O9.5Vep | [79] | 18.0 | [73] | 9.6 | [80] | 0.3 | [80] | 2005653524280214400 |
| SAX J2239.3+6116(g) | Be | B0Ve | [81] | 17.5 | [9] | 262.0 | [82] | – | – | 2201091578667140352 |
Notes. Systems with a measured pulse-period according to: (a)Uchida et al. (2021), (b)Sanjurjo-Ferrrín et al. (2017), (c)Staubert et al. (2019), (d)Walter et al. (2015), (e)Weng et al. (2022), (f)La Palombara & Mereghetti (2017), (g)van den Eijnden et al. (2021), (h)Pradhan et al. (2013), (i)Kabiraj & Paul (2020). Companion masses with no uncertainty provided come from photometric masses taken from [9] or [73]; a 20% systematic error is assumed in the rest of the paper. This table is available online at https://apc.u-paris.fr/~fortin/HMXB_catalogue.html and at the CDS alongside other HMXBs detected by Gaia that did not meet the quality criteria for this study.
References. [1] Reig et al. (2005a); [2] Grunhut et al. (2014); [3] in’t Zand et al. (2007); [4] Krtička et al. (2015); [5] Hu et al. (2017); [6] Crampton et al. (1985); [7] Koenigsberger et al. (2006); [8] Negueruela & Okazaki (2001); [9] Porter (1996); [10] Raichur & Paul (2010); [11] Corbet & Krimm (2010); [12] Kaur et al. (2008); [13] Hutchings et al. (1981); [14] Casares et al. (2005a); [15] Gregory (2002); [16] Aragona et al. (2009); [17] Negueruela et al. (1999); [18] Martins et al. (2005); [19] Slettebak (1982); [20] Lyubimkov et al. (1997); [21] Delgado-Martí et al. (2001); [22] Hynes et al. (2002); [23] Reig et al. (2005b); [24] Ferrigno et al. (2013); [25] Polcaro et al. (1990); [26] Wang & Gies (1998); [27] Okazaki & Negueruela (2001); [28] Finger et al. (1996); [29] Jaschek & Egret (1982); [30] Aragona et al. (2010); [31] Moritani et al. (2018); [32] Kaaret et al. (1999); [33] Kaaret et al. (2000); [34] Masetti et al. (2010); [35] Sota et al. (2014); [36] Gamen et al. (2015); [37] Houk (1978); [38] Falanga et al. (2015); [39] Stickland et al. (1997); [40] Coe et al. (1994); [41] Sidoli & Paizis (2018); [42] Strader et al. (2015); [43] Waisberg & Romani (2015) & Strader et al. (2015); [44] An et al. (2015); [45] Janot-Pacheco et al. (1981); [46] Walter et al. (2015); [47] Densham & Charles (1982); [48] Hutchings et al. (1987); [49] Ray & Chakrabarty (2002); [50] Pacheco et al. (1982); [51] Masetti et al. (2009); [52] Hutchings et al. (1982); [53] Kaper et al. (2006); [54] Parkes et al. (1980); [55] Negueruela et al. (2011); [56] Miller-Jones et al. (2018); [57] Masetti et al. (2008); [58] Parkes et al. (1978); [59] Abubekerov et al. (2004); [60] Vieira et al. (2003); [61] Coleiro et al. (2013); [62] Nespoli et al. (2008); [63] Islam & Paul (2016); [64] Lopes de Oliveira et al. (2006); [65] Pellizza et al. (2006); [66] Bikmaev et al. (2017); [67] Nikolaeva et al. (2013); [68] Townsend et al. (2011); [69] Casares et al. (2005b); [70] Casares et al. (2011); [71] Negueruela et al. (2008); [72] Coe et al. (1988); [73] Zorec et al. (2005); [74] Wilson et al. (1998); [75] Reig et al. (2004); [76] Baykal et al. (2007); [77] Bonnet-Bidaud & Mouchet (1998); [78] McBride et al. (2007); [79] Blay et al. (2006); [80] Stoyanov et al. (2014); [81] Reig et al. (2017); [82] in’t Zand et al. (2000).
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