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Table B.2

Main observational properties.

(D ID (2) Type (3) Name (4) P/T (5) Accretor (6) Porb (min) (7) FX [2–10 keV] (erg cm−2 s−1) (8) mag (9) Nн (×1022 cm−2) (10) GC E(B – V) (mag) (11) References
1 UCXB 4U 1820-303 (NGC 6624) Ρ NS 11.42 5.02×10−09 B=18.7 0.16±0.003 0.28 ± 0.03 Stella et al. (1987)p. Costantini et al. (2012)F, King et al. (1993)m·
Sidoli et al. (2001)N, Harris (2010)E
2 UCXB 4U 0513-40 (NGC 1851) Ρ NS 17 1.33×10−10 B=21.1 0.026 0.02±0.01 Zurek et al. (2009)p.Fiocchi et al. (20U)F,Deutsch et al. (1996)m
Sidoli et al. (2001)N, Harris (2010)E
3 UCXB 2S 0918-549 Ρ NS 17.4 1.12×10−10 V = 20.98±0.07 0.3 Zhong & Wang (2011)p, Juett & Chakrabarty (2003)F, Chevalier & Ilovaisky (1987)m
Juett & Chakrabarty (2003)N
4 UCXB 4U 1543-624 Ρ NS 18.2 7.27×10−10 r’ =20.42±0.03 0.35 Wang & Chakrabarty (2004)p,Juett & Chakrabarty (2003)F,Wang & Chakrabarty (2004)m
Juett & Chakrabarty (2003)N
5 UCXB 4U 1850-087 (NGC 6712) Ρ NS 20.6 1.04×10−10 B=21.2±0.2 0.4±0.2 0.45±0.04 Homer et al. (1996)p,Juett & Chakrabarty (2005)F,Auriere & Koch-Miramond (1992)m
Sidoli et al. (2006)N,Harris (2010)E
6 UCXB M15 X-2 (M15/NGC 7078) Ρ NS 22.5806 6.71×10−11 U=18.6 <0.034 0.1 ±0.01 Dieball et al. (2005)p,White & Angelini (2001)F,de Marchi & Paresce (1994); White & Angelini (2001)m
White & Angelini (2001)N,Harris (2010)E
7 UCXB 47 Tuc X-9 (47 Tuc/NGC 104) Ρ 28.18 4.73×10−12 U=19.4 0.013 0.04±0.02 Bahramian et al. (2017)p,Bahramian et al. (2017)F,Paresce et al. (1992)m
Heinke et al. (2005)N,Harris (2010); Salaris et al. (2007)E
8 UCXB IGR J17062-6143 P(QP) NS(AMXP) 37.9701 5.53×10−11 g’=20.23±0.16 0.26 Strohmayer et al. (2018a)p,Keek et al. (2017)F,Hernández Santisteban et al. (2019)m
Degenaar et al. (2017)N
9 UCXB XTE J1807-294 Τ NS(AMXP) 40.0741 1.19×10−10 qV>24.3 Markwardt et al. (2003a)p,Campana et al. (2003)F,D’Avanzo et al. (2009)m
Campana et al. (2003)N
10 UCXB 4U 1626-67 Ρ NS 41.538 2.96×10−10 V=18.54±0.11 Middleditch et al. (1981)p,Hemphill et al. (2021)F,McClintock et al. (1977)m
Krauss et al. (2007)N
11 UCXB XTE J1751-305 T NS(AMXP) 42.42235 1.27×10−09 R>23.l Markwardt et al. (2002)p,Gierliński & Poutanen (2005)F,Jonker et al. (2003b)m
Gierliński & Poutanen (2005)N
12 UCXB XTE J0929-314 T NS(AMXP) 43.57910 2.70×10−10 V=18.63±0.03 0.076 Galloway et al. (2002)p,Juett et al. (2003)F,Giles et al. (2005); Monelli et al. (2005)m
qV=27.58±0.12 Juett et al. (2003)N
13 UCXB MAXI J0911-655 (NGC 2808) T NS(AMXP) 44.332218 1.37×10−10 0.25±0.01 0.22±0.02 Sanna et al. (2017)p,Sanna et al. (2017)F
Sanna et al. (2017)N,Harris (2010)E
14 UCXB IGR J16597-3704 (NGC 6256) Τ NS(AMXP) 45.97 1.97×10−10 0.82±0.10 1.09±0.11 Sanna et al. (2018a)p, Sanna et al. (2018a)F
Sanna et al. (2018a)N,Harris (2010)E
15 UCXB 4U 1916-053 Ρ NS 49.75 5.57×10−10 V=20.99±0.05, 0.55±0.04 Walter et al. (1982); White & Swank (1982)p Jaria et al. (2006)F,Grindlay et al. (1987)m
Iaria et al. (2021)N
16 UCXB 4U 0614+091 Ρ NS 51.3 1.77×10−09 V = 18.87±0.08 0.3 Shahbaz et al. (2008)p,Lin & Yu (2018)F,Machin et al. (1990)m
Madej et al. (2010)N
17 UCXB Swift J1756.9-2508 T NS(AMXP) 54.7017 1.54×10−09 Krimm et al. (2007)p,Sanna et al. (2018c)F
Sanna et al. (2018с)N
18 UCXB NGC 6440 X-2 (NGC 6440) T NS(AMXP) 57.3 1.58×10−10 g’>22 0.69±0.06 1.07±0.10 Altamirano et al. (2010)p,Heinke et al. (2009)F,Heinke et al. (2009)m
qV>21.0 Heinke et al. (2009)N,Harris (1996)E
19 UCXB MAXI J1957+032 T NS(AMXP ) 60.8841 4.91×10−10 R=18.27±0.06 0.17 Sanna et al. (2022)p,Mata Sánchez et al. (2017)F,Guver et al. (2015); Mata Sánchez et al. (2017)m
qR=21.4±0.2 Mata Sánchez et al. (2017)N
20 UCXB IGR J17494-3030 T NS(AMXP) 74.9445 9.35×10−11 1.87 Ng et al. (2021)p Armas Padilla et al. (2013b)F
Armas Padilla et al. (2013b)N
21 spLMXB HETE J1900.1-2455 T(LO) NS(AMXP ) 83.2543 3.92×10−10 V=18.09±0.03 0.105 Kaaret et al. (2006)p,Papitto et al. (2013)F,Steeghs et al. (2005)m
Papitto et al. (2013)N
22 spLMXB 1E 1603.6+2600 Ρ NS 111.04 4.1·9×10−12 R=19.4 0.15±0.03 Morris et al. (1990)p,Jonker et al. (2003c)F.Morris et al. (1990)m
Jonker et al. (2003с)N
23 spLMXB IGR J17379-3747 T NS(AMXP) 111.65 1.23×10−10 R=21.5±0.3 0.90±0.03 Sanna et al. (2018b); Strohmayer et al. (2018b)p,van den Eijnden et al. (2018b)F,Curran et al. (2011)m
Sanna et al. (2018b)N
24 spLMXB 4U 1812-12 Ρ NS 114 3.80×10−10 r=22.7 1.50 Armas Padilla et al. (2022)p,Muno et al. (2005)F,Armas Padilla et al. (2020)m
Tarana et al. (2006); Barret et al. (2003)N
25 cUCXB 4U 1728−34 Ρ NS 2.08×10−09 K=15.1 4.5±0.1 Wang et al. (2019)F,Martí et al. (1998)m
Wang et al. (2019)N
26 cUCXB NGC 6652 В (NGC 6652) Τ NS 7.52×10−13 В = 20.4 0.05 0.09±0.01 Stacey et al. (2012)F, Deutsch et al. (1998)m
Coomber et al. (2011)N,Harris (2010)E
27 cUCXB 4U 1822−00 Ρ NS 5.80×10−10 r'=21.58±0.08 0.97±0.18 Hertz & Grindlay (1984)F,Wang & Chakrabarty (2004)m
Juett & Chakrabarty (2005)N
28 cUCXB 4U 1905+000 T(LO) NS 1.57×10−10 V = 20.5±0.04 0.3±0.1 Christian & Swank (1997)F .Chevalier et al. (1985)m·
Chevalier et al. (1990)N
29 cUCXB RX J1709.5−2639 (NGC 6293) Τ NS 9.10×10−10 R=20.5±0.1 0.29±0.01 1.36±0.04 Ludlam et al. (2017)F,Jonker et al. (2004)m
qR=22.24±0.03 Degenaar et al. (2013)N,Harris (2010)E
30 cUCXB АХ J1754.2−2754 P(QP) NS 9.55×10−12 Ks=18.12±0.15 2.93±0.06 Armas Padilla et al. (2013a)F,Shaw et al. (2017)m
Armas Padilla et al. (2013а)N
31 cUCXB 1RXS J171824.2−402934 Ρ NS 3.75×10−12 1.9±0.1 Armas Padilla et al. (2013a)F
Armas Padilla et al. (2013а)N
32 cUCXB 1RXH J173523.7−354013 Ρ NS 2.30×10−12 V=21.2 1.4±0.1 Armas Padilla et al. (2013a)F,Degenaar et al. (2010)m
Armas Padilla et al. (2013а)N
33 cUCXB XMMU J174716.1−281048 T(LO) NS 6.40×10−12 H=15.3±0.1 8.9±0.5 Degenaar et al. (2011)F,Degenaar et al. (2007)m
Del Santo et al. (2007)N
34 cUCXB SAX J1806.5−2215 T(LO) NS 6.60×10−10 K=17.25±0.03 4.2±0.6 Del Santo et al. (2012)F,Kaur et al. (2017)m
qK>18.2 Del Santo et al. (2012)N
35 cUCXB AХ J1538.3−5541 P(QP) 2.57×10−11 K=18 7.7±0.5 Degenaar et al. (2012b)F,Anderson et al. (2014)m
Degenaar et al. (2012b)N
36 cUCXB Swift J0840.7−3516 Τ 9.91×10−10 R=16.3±0.1 Coti Zelati et al. (2021)F,Melandri et al. (2020); Coti Zelati et al. (2021)m
qr=21 Coti Zelati et al. (2021)N
37 cUCXB 1A 1246−588 Ρ NS 9.10×10−11 V=19.45 0.5 in ’t Zand et al. (2008)F.Bassa et al. (2006)m
in ’t Zand et al. (2008)N
38 cUCXB SAX J1712.6−3739 Ρ NS 1.29×10−10 V=23.93±0.26 1.3 Lin & Yu (2020)F,Wiersema et al. (2009)m
Fiocchi et al. (2008)N
39 cUCXB 1RXS J170854.4−321857 P(QP) NS 4.57×10−11 K > 20.1 0.34±0.04 Armas Padilla & López-Navas (2019)F .Revnivtsev et al. (2013)N
Armas Padilla & López-Navas (2019)N
40 cUCXB 4U 1722−30 (Terzan 2) Ρ NS 5.74×10−10 1.1 1.87±0.19 Lin & Yu (2018)F
Kashyap et al. (2022)N,Harris (2010); Valenti et al. (2010)E
41 cUCXB IGR J17254−3257 Ρ NS 2.77×10−11 1.79 Chenevez et al. (2007)F
Chenevez et al. (2007)N
42 cUCXB SLX 1735−269 Ρ NS 3.45×10−10 R=21.31±0.12 l.70±0.05 Wilson et al. (2003)F,Zolotukhin & Revnivtsev (2011)m
Wilson et al. (2003)N
43 cUCXB SLX 1737−282 Ρ NS 5.53×10−11 1.9+/−0.1 Armas Padilla et al. (2018)F
Armas Padilla et al. (2018); in ’t Zand et al. (2002)N
44 cUCXB SLX 1744−299 Ρ NS 2.08×10−10 I=23.37±0.28 3.5 Mori et al. (2005)F,Zolotukhin & Revnivtsev (2011)m
Mori et al. (2005)N
45 cUCXB 1RXS J180408.9−342058 T NS 1.97×10−09 V=17.71±0.02 0.48+/−0.02 Degenaar et al. (2016)F,Baglio et al. (2016)m
Degenaar et al. (2016)N
46 cUCXB IGR J17285−2922 T 1.04×10−10 1=18.24 0.99+/−0.05 Stoop et al. (2021)F,Stoop et al. (2021)m
Stoop et al. (2021)N
47 cUCXB XMMU J181227.8−181234 T NS 2.85×10−09 12.8±0.3 Cackett et al. (2006)F
Cackett et al. (2006)N
48 cUCXB 1M 1716−315 T(LO) NS 1.07×10−09 I>23.5 0.21±0.06 Jonker et al. (2007)F,Jonker et al. (2007)m
Christian & Swank (1997)N
49 cUCXB 1A 1744−361 Τ NS 1.4×10−9 0.41 ±0.01 Gavriil et al. (2012)F
Gavriil et al. (2012)N

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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