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Table B.3

Additional multi-wavelength properties.

(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)
ID Type Name short-B IB SB X-ray Optical UV Lo/LX< < LXPers ≪ References
1 UCXB 4U 1820−303 (NGC 6624) ✓ ✓ −O VII, −O VIII, −Ne IX Clark et al. (1977)B, Strohmayer & Brown (2002)SB
Futamoto et al. (2004); Cackett et al. (2008)X
2 UCXB 4U 0513−40 (NGC 1851) ✓ −0 ✓ Forman & Jones (1976); Galloway et al. (2020)B
Juett & Chakrabarty (2005)X, Deutsch et al. (2000)o/x
3 UCXB 2S 0918−549 ✓ ✓ Ne Featureless ✓ У Jonker et al. (2001)B,in ’t Zand et al. (2005)IB,Juett et al. (2001)X
Nelemans et al. (2004, 2006)o,Juett et al. (2001)o/x
Jonker et al. (2001)Lp
4 UCXB 4U 1543−624 ✓ Ne/O +C, +O ✓ У Serino et al. (2018)B,Juett & Chakrabarty (2OO3)X,Nelemans et al. (2004)o
Juett et al. (2001)o/x,Wang & Chakrabarty (2004)Lp
5 UCXB 4U 1850−087 (NGC 6712) ✓ ✓ Ne Featureless Featureless ✓ У Swank et al. (1976); Hoffman et al. (1980)Bin ’t Zand et al. (2014)IB
Juett et al. (2001)X
Auriere & Koch-Miramond (1992); Downes et al. (1996)o,uv
Juett et al. (2001)o/x ’t Zand et al. (2007)Lp
6 UCXB M 15 X−2 (M 15/NGC 7078) ✓ ✓ +C IV?,+He II? У van Paradijs et al. (1990); Smale (2001)BGalloway et al. (2020)IB
Dieball et al. (2005)uv,in ’t Zand et al. (2007)Lp
7 UCXB 47 Tuc X-9 (47 Tuc/NGC 104) +O VII, +O VII Featureless +C IV У Heinke et al. (2005); Bahramian et al. (2017)X
Bump at ~O.3 keV Tudor et al. (2018)oKnigge et al. (2008)uv
Bahramian et al. (2017); Bahramian & Degenaar (2023)Lp
8 UCXB IGR J17062−6143 ✓ ✓ +O Featureless У Degenaar et al. (2012a)IB, Negoro et al. (2015b)SB
Absorption at ~3.4 keV (Ce ι or Ti) van den Eijnden et al. (2018a); Bult et al. (2021)X
Hernández Santisteban et al. (2019)o ,Degenaar et al. (2017)Lp
9 UCXB XTE J1807−294
10 UCXB 4U 1626−67 +Ne X, +Ne IX, +O VII, +C, +0 Lyα, С III, O IV, Ο V, Angelini et al. (1995); Schulz et al. (2001); Krauss et al. (2007)X
+O VII, +Fe-L Si IV, С IV, О III Werner et al. (2006); Nelemans et al. (2006)oHomer et al. (2002)uv
11 UCXB XTE J1751−305
12 UCXB XTE J0929−314 −O Emission at -4640/1 Juett et al. (2003)X ,Nelemans et al. (2006)o
(C or N)
13 UCXB MAXI J0911−655 (NGC 2808) ✓ Nakajima et al. (2020)IB
14 UCXB IGR J16597−3704 (NGC 6256)
15 UCXB 4U 1916−053 ✓ −Ne X, -Mg XII, -Si XIV, He I, He II, Ν II, Ν III У Becker et al. (1977)B
−S XVI, −O VIII, −Ca XX Iaria et al. (2006); Gambino et al. (2019); Iaria et al. (2021)X
Nelemans et al. (2006)o,in ’t Zand et al. (2007)Lp
16 UCXB 4U 0614+091 ✓ ✓ ✓ Ne, O +C, +O, +N Featureless ✓ У Lewin (1976)BKuulkers et al. (2010)IB
Kuulkers (2005)S BJuett et al. (2001); Madej et al. (2010)X
Machin et al. (1990); Nelemans et al. (2004); Madej et al. (2013)o
Madej et al. (2013)uv Juett et al. (2001)o/x ’t Zand et al. (2007)Lp
17 UCXB Swift J1756.9−2508
18 UCXB NGC 6440 X−2 (NGC 6440)
19 UCXB MAXI J1957+032 Featureless Mata Sánchez et al. (2017)o
20 UCXB IGR J17494−3030
21 spLMXB HETE J1900.1−2455 ✓ Excess at ∼1 keV + Hα, +He II Vanderspek et al. (2005); Galloway et al. (2020)B
(Fe-Lα and/or Ne-Kα) Bowen blend of N III and С III Papitto et al. (2013)X,Elebert et al. (2007); Steeghs et al. (2005)o
22 spLMXB 1E 1603.6+2600 ✓ Emission at ∼0.5 keV and ~0.65 keV +Hα, +Нβ +He II У Mukai et al. (2001)B,Hakala et al. (2005)BX
(N VII and/or O VIII) −He I, −Ca II Morris et al. (1990)o,in ’t Zand et al. (2007)Lp
23 spLMXB IGR J17379−3747 ✓ Chelovekov et al. (2006); Chelovekov & Grebenev (2010)B
24 spLMXB 4U 1812−12 ✓ Featureless ✓ ✓ Murakami et al. (1983); Galloway et al. (2020)B
Armas Padilla et al. (2022)o,Bassa et al. (2006)o/x
in ’t Zand et al. (2007)Lp
25 cUCXB 4U 1728−34 ✓ +Mg XI, emission at ~0.5 keV Hoffman et al. (1976); Galloway et al. (2010)B
Absorption at ∼0.7 keV Di Salvo et al. (2000); Koliopanos et al. (2021)X
26 cUCXB NGC 6652 В (NGC 6652) ✓ + H,+He in ’t Zand et al. (1998)B,Paduano et al. (2021)o
−Fe, −Mg, −Na, −О
27 cUCXB 4U 1822−00 ✓ Featureless ✓ Asai et al. (2016)B,Nelemans et al. (2006)o
Juett & Chakrabarty (2005)o/x
28 cUCXB 4U 1905+000 ✓ ✓ Lewin et al. (1976)B ,Chevalier et al. (1990)o/x
29 cUCXB RX J1709.5−2639 (NGC 6293) ✓ Emission at ∼0.6 keV Cocchi et al. (1998)B, Jonker et al. (2003a)X
(O and/or Fe, enhanced Ne/O)
30 cUCXB AХ J1754.2−2754 ✓ ✓ ✓ ✓ Chelovekov & Grebenev (2007)BChenevez et al. (2017)IB
Bassa et al. (2OO8)o/xBassa et al. (2008)Lp
31 cUCXB 1RXS J171824.2−402934 ✓ ✓ Kaptein et al. (2000)B ,in ’t Zand et al. (2005)Lp
32 cUCXB 1RXH J173523.7−354013 ✓ + Hα, +Ca II, +O I ✓ Degenaar et al. (2010)IB,o,Lp,Armas Padilla et al. (2013a)Lp
33 cUCXB XMMU J174716.1−281048 ✓ ✓ Brandt et al. (2006b)BDegenaar et al. (2011)IB
34 cUCXB SAX J1806.5−2215 ✓ ✓ ✓ Cornelisse et al. (2002)B,Lp,in ’t Zand et al. (2019)IB
35 cUCXB AХ J1538.3−5541
36 cUCXB Swift J0840.7−3516 Absorption at ∼3.4 keV Blend of С and О in emission, Shidatsu et al. (2021)X,Coti Zelati et al. (2021)o
(Fe K?) + He I, +C II
37 cUCXB 1A 1246−588 ✓ ✓ −О, −Ne, −Fe Featureless ✓ ✓ Boller et al. (1997); Piro et al. (1997)B,in ’t Zand et al. (2008)IB
in ’t Zand et al. (2008)X,in ’t Zand et al. (2008)o
Bassa et al. (2006)o/x,in ’t Zand et al. (2007)Lp
38 cUCXB SAX J1712.6−3739 ✓ ✓ ✓ Cocchi et al. (1999)B,Kuulkers (2009)IB,in ’t Zand et al. (2007)Lp
39 cUCXB 1RXS J170854.4−321857 ✓ Overabundances of Ne and Fe ✓ in ’t Zand et al. (2004, 2005)IB
at ~1 keV Armas Padilla & López-Navas (2019)X ,in ’t Zand et al. (2007)Lp
40 cUCXB 4U 1722−30 (Terzan 2) ✓ ✓ Swank et al. (1977); Kuulkers et al. (2003)B
in ’t Zand et al. (2007)Lp
41 cUCXB IGR J17254−3257 ✓ ✓ ✓ Brandt et al. (2006a)BChenevez et al. (2007)IB
in ’t Zand et al. (2007)Lp
42 cUCXB SLX 1735−269 ✓ ✓ ✓ ✓ Bazzano et al. (1997)BMolkov et al. (2005)IB
Suzuki & Kawai (2005)SB ,in ’t Zand et al. (2007)Lp
43 cUCXB SLX 1737−282 ✓ ✓ in ’t Zand et al. (2002); Falanga et al. (2008)IB
in ’t Zand et al. (2007)Lp
44 cUCXB SLX 1744−299 ✓ ✓ Pavlinsky et al. (1994); in ’t Zand et al. (2007); Alizai et al. (2020)IB
in ’t Zand et al. (2007)Lp
45 cUCXB 1RXS J180408.9−342058 ✓ +NVII, +0 VII, + O VIII + He II Chenevez et al. (2012); Wijnands et al. (2017)B
Ludlam et al. (2016); Degenaar et al. (2016)X.Baglio et al. (2016)o
46 cUCXB IGR J17285−2922 Negative residuals at ≤1 keV Featureless Sidoli et al. (2011)X,Stoop et al. (2021)o
47 cUCXB XMMU J181227.8−181234 ✓ Goodwin et al. (2019)B
48 cUCXB 1M 1716−315 ✓ ✓ Hoffman et al. (1978)B,Markert et al. (1976); Tawara et al. (1984)IB
49 cUCXB 1A 1744−361 ✓ Emelyanov et al. (2001); Bhattacharyya et al. (2006)B

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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