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Table B.1

Astrometry and location.

(1) ID (2) Type (3) Year (4) Name (GC) (5) RA (h m s) (6) Dec (º ′ ″) (7) Error a (″) (8) ℓ (º) (9) b (º) (10) db (kpc) (11) z (kpc) (12) References
1 UCXB 1972 4U 1820-303 (NGC 6624) 18:23:40.50 −30:21:40.09 (r) 0.0004,0.005 2.788211 −7.913491 8.019 −1.101 Giacconi et al. (1972)y, Díaz Trigo et al. (2017)c
Baumgardt & Vasiliev (2021)d
2 UCXB 1972 4U 0513-40 (NGC 1851) 05:14:06.40 −40:02:38 (o) 0.7 244.509804 −35.036749 11.951 −6.889 Forman & Jones (1976)y, Homer et al. (2001)c
Baumgar dt & Vasiliev (2021)d
3 UCXB 1974 2S 0918-549 09:20:26.95 −55:12:24.7 (x) 0.6 275.852936 −3.844515 3.0 (H), 3.9 (He) −0.261 Giacconi et al. (1974)y, Juett & Chakrabarty (2003)c
Galloway et al. (2020)d
4 UCXB 1972 4U 1543-624 15:47:54.69 −62:34:05.4 (x) 0.6 321.756967 −6.336329 9.2 (He) −1.015 Giacconi et al. (1972)y, Juett & Chakrabarty (2003)c
Serino et al. (2018)d
5 UCXB 1975-1976 4U 1850-087 (NGC 6712) 18:53:04.88 −08:42:20.0 (r) 0.4 25.355515 −4.319866 7.382 −0.557 Seward et al. (1976a); Swank et al. (1976)y, Lehto et al. (1990)c
Baumgardt & Vasiliev (2021)d
6 UCXB 2000 M15X-2(M15/NGC 7078) 21:29:58.14 +12:10:01.52 (uv) 65.012156 −27.311977 10.709 −4.910 White & Angelini (2001)y, Haurberg et al. (2010)c
Baumgardt & Vasiliev (2021)d
7 UCXB 1981 47 Tue X-9 (47 Tuc/NGC 104) 00:24:04.25 −72:04:58.02 (x) 0.001, 0.01 305.89703 −44.887576 4.521 −3.176 Grindlay (1981)y, Heinke et al. (2005)c
Baumgardt & Vasiliev (2021)d
8 UCXB 2006 IGR J17062-6143 17:06:16.3 −61:42:40.5 (uv) 0.3 328.719432 −12.398127 7.3 (He) −1.567 Churazov et al. (2007)y, Ricci et al. (2008)c
Keek et al. (2017)d
9 UCXB 2003 XTE J1807-294 18:06:59.8 −29:24:30 (X)1 1.935298 −4.272579 assumed 8 −0.596 Markwardt et al. (2003b)y, Markwardt et al. (2003a)c
Campana et al. (2003)d
10 UCXB 1972 4U 1626-67 16:32:16.79 −67:27:39.3 (X) 321.788351 −13.091711 8 −1.812 Giacconi et al. (1972)y , Lin et al. (2012)c
Chakrabarty (1998)d
11 UCXB 2002 XTE J1751-305 17:51:13.49 −30:37:23.4 (x) 0.05, 0.6 359.181912 −1.912008 assumed 8.5 −0.284 Markwardt et al. (2002)y, Markwardt et al. (2002)c
Gierliński & Poutanen (2005)d
12 UCXB 2002 XTE J0929-314 09:29:20.19 −31:23:03.2 (o) 0.1 260.105098 14.214563 assumed 10 2.456 Remillard & RXTE ASM Team (2002)y, Giles et al. (2005)c
Campana et al. (2005)d
13 UCXB 2016 MAXI J0911-655 (NGC 2808) 09:12:02.43 −64:52:06.4 (x) 0.6 282.195949 −11.256788 10.060 −1.952 Serino et al. (2016)y, Homan et al. (2016)c
Baumgardt & Vasiliev (2021)d
14 UCXB 2017 IGR J16597-3704 (NGC 6256) 16:59:32.90 −37:07:14.28 (r) 0.005,0.22 347.792766 3.306254 7.242 0.415 Bozzo et al. (2017)y, Tetarenko et al. (2018)c
Baumgardt & Vasiliev (2021)d
15 UCXB 1972 4U 1916-053 19:18:47.87 −05:14:17.09 (x) 0.6 31.357765 −8.463592 5.8(H), 7.6(He) −1.119 Giacconi et al. (1972)y, Iaria et al. (2006)c
Galloway et al. (2020)d
16 UCXB 1972 4U 0614+091 06:17:07.35 +09:08:13.4 (r) 0.1 200.877357 −3.363284 l.99(H),2.59(He) −0.153 Giacconi et al. (1972)y, Migliari et al. (2010)c
Galloway et al. (2020)d
17 UCXB 2007 Swift J1756.9-2508 17:56:57.43 −25:06:27.4 (x) 0.5 4.580765 −0.212396 assumed 8 −0.030 Krimm et al. (2007)y, Sanna et al. (2018c)c
Krimm et al. (2007)d
18 UCXB 2009 NGC 6440 X-2 (NGC 6440) 17:48:52.76 −20:21:24.0 (x) 0.02,0.1 7.731804 3.802875 8.248 0.544 Heinke et al. (2009)y, Heinke et al. (2009)c
Baumgardt & Vasiliev (2021)d
19 UCXB 2015 MAXI J1957+032 19:56:39.11 +03:26:43.66 (x) 0.6 43.645509 −12.825722 5 −1.110 Negoro et al. (2015a); Cherepashchuk et al. (2015)y, Chakrabarty et al. (2016)c
Mata Sánchez et al. (2017); Ravi (2017)d
20 UCXB 2012 IGR J17494-3030 17:49:23.62 −30:29:59.0 (x) 0.6 359.086011 −1.510211 assumed 8 −0.211 Boissay et al. (2012)y, Chakrabarty & Jonker (2020)c
Armas Padilla et al. (2013b)d
21 spLMXB 2005 HETE J1900.1-2455 19:00:09.77 −24:54:04 (r) 0.1,0.1 11.324799 −12.868715 2.9(H), 3.8(He) −0.846 Vanderspek et al. (2005)y, Rupen et al. (2005)c
Galloway et al. (2020)d
22 spLMXB 1990 1E 1603.6+2600 16:05:45.87 +25:51:45.24 (G) 0.0001, 0.0002 42.750438 46.77836 2.1 Gaia 1.530 Gioia et al. (1990)y, Brown et al. (2021); Morris et al. (1990)c
Arnason et al. (2021)d
23 spLMXB 2004 IGR J17379-3747 17:37:58.84 −37:46:18.35 (r) 0.02, 0.07 351.648136 −3.305259 assumed 8.5 −0.490 Chelovekov et al. (2006)y, Van Den Eijnden et al. (2021)c
Chelovekov et al. (2006)d
24 spLMXB 1972 4U 1812-12 18:15:06.15 −12:05:46.7 (o) 0.19, 0.21 18.032721 2.397809 2.3(H)-3(He) 0.096 Giacconi et al. (1972)y, Bassa et al. (2006)c Galloway et al. (2020)d
25 cUCXB 1972 4U 1728-34 17:31:57.68 −33:50:01.54 (r) 0.0003, 0.005 354.303524 −0.150417 3.3(H), 4.4 (He); −0.012 Giacconi et al. (1972)y, Díaz Trigo et al. (2017)c Galloway et al. (2020)d
26 cUCXB 1998 NGC 6652 В (NGC 6652) 18:35:44.54 −32:59:38.97 (x) 0.009, 0.09 1.529081 −11.37483 9.464 −1.874 Deutsch et al. (1998); Heinke et al. (2001)y, Heinke et al. (2001)c Baumgardt & Vasiliev (2021)d
27 cUCXB 1972 4U 1822-00 18:25:22.02 −00:00:43.0 (x) 0.6 29.939078 5.792617 13 1.312 Giacconi et al. (1972)y, Juett & Chakrabarty (2005)c Asai et al. (2016)d
28 cUCXB 1976 4U 1905+000 19:08:26.97 +00:10:07.7 (o) 35.024458 −3.707147 7.5 (H), 10 (He) −0.647 Seward et al. (1976a); Villa et al. (1976)y, Gottwald et al. (1991)c Jonker & Nelemans (2004)d
29 cUCXB 1990 RX J1709.5-2639 (NGC 6293) 17:09:30.4 −26:39:19.9 (x) 0.6 357.472538 7.911726 9.192 1.266 Voges et al. (1999)y, Jonker et al. (2003a)c Baumgardt & Vasiliev (2021)d
30 cUCXB 1999 АХ J1754.2-2754 17:54:14.5 −27:54:35.6 (x) 0.45 1.853974 −1.099765 6.6(H),9.2(He) −0.177 Sakano et al. (2002)y, Bassa et al. (2008)c Chelovekov & Grebenev (2007)d
31 cUCXB 1990 1RXS J171824.2-402934 17:18:24.14 −40:29:33.04 (x) 0.6 347.276837 −1.651634 4.7(H),6.1(He) −0.176 Voges et al. (1999)y, in ’t Zand et al. (2005)c Galloway et al. (2020)d
32 cUCXB 1990 1RXH J173523.7-354013 17:35:23.75 −35:40:16.1 (uv) 0.56 353.144504 −1.741226 6.2(H),9.5(He) −0.289 Voges et al. (1999)y, Israel et al. (2008)c Degenaar et al. (2010)d
33 cUCXB 2003 XMMU J174716.1-281048 17:47:16.16 −28:10:48.0 (x) 0.5 0.834266 0.083421 <5.3 (H),<8.4 (He) 0.012 Sidoli & Mereghetti (2003)y, Degenaar et al. (2007)c Degenaar et al. (2011)d
34 cUCXB 1996-1997 SAX J1806.5-2215 18:06:32.17 −22:14:17.32 (i) 0.03, 0.05 8.159359 −0.699213 <4.8 (H),<6.2 (He) −0.076 in ’t Zand et al. (1999b)y, Kaur et al. (2017)c Galloway et al. (2020)d
35 cUCXB 1998 АХ J1538.3-5541 15:38:14.00 −55:42:13.6 (x) 0.8 324.945782 −0.130139 assumed 8 −0.018 Sugizaki et al. (2001); Degenaar et al. (2012b)y, Anderson et al. (2014)c Degenaar et al. (2012b)d
36 cUCXB 2020 Swift J0840.7-3516 08:40:40.94 −35:16:25.1 (o) 0.2 256.281083 4.017002 assumed 8 0.560 Evans et al. (2020)y, Malesani et al. (2020)c Coti Zelati et al. (2021)d
37 cUCXB 1976 1A 1246-588 12:49:39.36 −59:05:14.68 (o) 0.06, 0.05 302.702563 3.783544 3.0 (H), 3.8 (He) 0.251 Seward et al. (1976b)y, Bassa et al. (2006)c Galloway et al. (2020)d
38 cUCXB 1999 SAX J1712.6-3739 17:12:36.77 −37:38:41.0 (x) 0.6 348.93894 0.919334 3.7(H), 4.8(He) 0.077 in ‘t Zand et al. (1999a)y, Wiersema et al. (2009)c Galloway et al. (2020)d
39 cUCXB 1972 1RXS J170854.4-321857 17:08:54.27 −32:19:57.13 (x) 0.6 352.780023 4.671897 <4.4(H), <5.7(He) 0.464 Giacconi et al. (1972)y, in ’t Zand et al. (2005)c Galloway et al. (2020)d
40 cUCXB 1975 4U 1722-30 (Terzan 2) 17:27:33.15 −30:48:07.8 (x) 0.6 356.319615 2.298083 7.753 0.313 Swank et al. (1977)y, Revnivtsev et al. (2002)c Baumgardt & Vasiliev (2021)d
41 cUCXB 2003 IGR J17254-3257 17:25:24.8 −32:57:15 (x) 2 354.279061 1.47467 <I4.5 (He) 0.373 Walter et al. (2004)y, Chenevez et al. (2007)c Chenevez et al. (2007)d
42 cUCXB 1985 SLX 1735-269 17:38:17.12 −26:59:38.6 (x) 0.6 0.796121 2.40017 4.5(H), 5.8(He) 0.243 Skinner et al. (1987)y, Wilson et al. (2003)c Galloway et al. (2020)d
43 cUCXB 1985 SLX 1737-282 17:40:42.83 −28:18:08.4 (x) 0.6 359.97359 1.249106 3.9(H), 5.l(He) 0.111 Skinner et al. (1987)y, Tomsick et al. (2007)c Galloway et al. (2020)d
44 cUCXB 1990 SLX 1744-299 17:47:25.89 −30:00:01.6 (o/i) 0.4 359.295259 −0.889669 <7.2 (H or He?) −0.112 Skinner et al. (1990)y, Zolotukhin & Revnivtsev (2011)c Chelovekov et al. (2017)d
45 cUCXB 1990 1RXS J180408.9-342058 18:04:08.37 −34:20:51.19 (r) 0.006,0.02 357.297382 −6.125046 <5.8 (He) −0.619 Voges et al. (1999)y, Deller et al. (2015)c Chenevez et al. (2012)d
46 cUCXB 2003 IGR J17285-2922 17:28:38.86 −29:21:44.0 (o) <O.l 357.651162 2.898254 assumed 8 0.405 Walter et al. (2004); Barlow et al. (2005)y, Torres et al. (2010)c Sidoli et al. (2011)d
47 cUCXB 2003 XMMU J181227.8-181234 18:12:27.8 −18:12:34 (x)2 12.357731 0.033671 20.9 (H), 27.2 (He) 0.016 Cackett et al. (2006)y, Cackett et al. (2006)c Galloway et al. (2020)d
48 cUCXB 1971-1974 1M 1716-315 17:18:47.02 −32:10:13.54 (x) 0.08,0.07 354.132917 3.069692 5.1 (H), 6.9 (He) 0.369 Markert et al. (1975)y, Jonker et al. (2007)c Jonker & Nelemans (2004)d
49 cUCXB 1976 1A 1744-361 17:48:13.15 −36:07:57.02 (r) 0.014, 0.30 354.119972 −4.192072 <7 (H), <9.1 (He) −0.665 Davison et al. (1976)y, Rupen et al. (2003)c Galloway et al. (2020)d

Notes. Columns: (1) ID number; (2) Source type; (3) Year of discovery; (4) preferred name of the system (GC if located in one); (5-7) Right ascension (RA) and declination (Dec) in equinox J2000, accuracy in the astrometry and source of the coordinates; (8-9) Galactic longitude (l) and latitude (b); (10–11) Estimated distance (d) and height above the Galactic plane (z); (12) References. (a)In Col. 7, the letter preceding the error value indicates the source of the coordinates: radio (r), optical (o), infrared (i), ultraviolet (uv), X-rays (x), Gaia (G), or a combination of them. If RA and Dec errors are different we give both. (b)We use the notation (H) and (He) for distances estimated using thermonuclear bursts, assuming hydrogen-rich and pure helium, respectively. (G) distances from Gaia parallaxes. For systems located in GCs, we report the distance to their host GC (see Sect. 3.1). In the References column (12), ‘y’ refers to discovery year, ‘c’ to coordinates, and ‘d’ to distance.

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