Table A.3
The dynamical BHs: photometric parameters in quiescence.
| Optical bands | NIR bands | |||||||
| NAME | Blue | Green | Red | Infrared | J | H | K/Ks | Ref. |
| (AB mag) | (AB mag) | (AB mag) | (AB mag) | (AB mag) | (AB mag) | (AB mag) | ||
|
|
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| Swift J1357.2–0933† | u′ = 23.12 ± 0.04 | g′ = 22.3 ± 0.4 | r′ = 21.5 ± 0.4 | i′ = 21.2 ± 0.4 | J = 20.51 ± 0.06 | H = 20.07 ± 0.05 | Ks = 20.09 ± 0.05 | Shahbaz et al. (2013) |
| g′ = 22.29 ± 0.08 | r′ = 21.71 ± 0.08 | Mata Sánchez et al. (2015); Armas Padilla et al. (2014) | ||||||
|
|
||||||||
| XTE J1650–500 | V ~ 24 | R ~ 22 | I> 19.3 | Garcia & Wilkes (2002); Curran et al. (2012) | ||||
|
|
||||||||
| XTE J1118+480 | B = 20.04 | V = 19.61 | R = 19.05 | J = 19.52 | H = 19.1 | Ks = 18.45 | Gelino et al. (2006) | |
| g′ = 21.0 ± 0.3 | i′ = 19.0 ± 0.2 | Shahbaz et al. (2005) | ||||||
|
|
||||||||
| XTE J1859+226 | V = 23.25 ± 0.09 | R = 22.54 ± 0.07 | Zurita et al. (2002) | |||||
| (V406 Vul) | J = 20.97 ± 0.03 | H = 20.68 ± 0.05 | Ks = 20.94 ± 0.35 | Gelino et al. (2010) | ||||
|
|
||||||||
| SAX J1819.3-2525 | B ~ 13.91 ± 0.04 | V ~ 13.66 ± 0.03 | I ~ 13.52 ± 0.03 | J = 14.86 ± 0.05 | H ~ 14.23 ± 0.05 | K ~ 12.83 ± 0.05∗ | MacDonald et al. (2014) | |
| (V4641 Sgr) | V = 13.96 ± 0.02 | R = 13.73 ± 0.02 | Orosz et al. (2001) | |||||
|
|
||||||||
| XTE J1550–564 | V = 22.0 ± 0.2 | i = 19.04 ± 0.03 | H = 17.6 ± 0.1 | Calvelo et al. (2010); Jain et al. (2001a) | ||||
| B> 23.8 ± 0.1 | V = 22.0 ± 0.4 | R ~ 22 | J = 19.24 ± 0.04 | Ks = 18.00 ± 0.04 | Orosz et al. (2002, 2011b) | |||
|
|
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| GRO J1655–40 | B ~ 18.5 | V ~ 17.5 | I ~ 15.4 | J ~ 14.76 | Ks ~ 15.12 | Greene et al. (2001) | ||
| (N. Sco 94) | B ~ 18.5 | V ~ 17.3 | R ~ 16.2 | I ~ 15.8 | Orosz & Bailyn (1997) | |||
| V = 17.3 ± 0.1 | R = 16.3 ± 0.1 | i = 14.9 ± 0.1 | van der Hooft et al. (1998) | |||||
|
|
||||||||
| GRS 1009-45 | V = 21.7 ± 0.2 | r = 20.4 ± 0.1 | Hynes et al. (2003a); Shahbaz et al. (1996) | |||||
| (N. Vel 93) | R = 21.3 ± 0.2 | Filippenko et al. (1999) | ||||||
|
|
||||||||
| GRS 1915+105 1 | J = 17.52 ± 0.08 1 | H = 13.09 1 | K = 11.4∗ 1 | Castro-Tirado et al. (1993); Shahbaz et al. (2008) | ||||
| (V1487 Aql) | I ~ 23.7 ± 0.4 1 | J = 18.72 ± 0.2 1 | H = 16.55 ± 0.04 1 | Ks = 15.28 ± 0.03 1 | Boeer et al. (1996); Eikenberry & Fazio (1995) | |||
|
|
||||||||
| GRO J0422+32 | V = 22.3 | R = 21.0 | I = 20.2 | Garcia et al. (1996) | ||||
| (V518 Per) | B = 23.1 ± 0.2 | V = 22.0 ± 0.1 | R = 21.0 ± 0.1 | I = 20.75 ± 0.08 | J = 19.3 ± 0.1 | H = 19.0 ± 0.2 | Ks = 19.29 ± 0.09 | Gelino & Harrison (2003); Webb et al. (2000) |
|
|
||||||||
| GRS 1124-684 | B = 22.6 ± 0.3 | V = 22.62 ± 0.03 | R = 19.8 ± 0.3 | I = 19.3 ± 0.2 | H ~ 18.39 | King et al. (1996b); Shahbaz et al. (1997) | ||
| (N. Mus 91) | u′ = 21.5 ± 0.4 | g′ = 20.65 ± 0.05 | i′ = 19.92 ± 0.04 | Shahbaz et al. (2010) | ||||
|
|
||||||||
| GS 2023+338 | B = 20.47 ± 0.05 | V = 18.38 ± 0.02 | R = 16.58 ± 0.01 | I = 16.07 ± 0.05 | J = 14.59 ± 0.08 | H = 14.21 ± 0.06 | Ks = 14.39 ± 0.05 | Casares et al. (1993); Zurita et al. (2004) |
| (V404 Cyg) | ||||||||
|
|
||||||||
| GS 2000+251 | R = 21.3 ± 0.2 | I = 20.2 ± 0.2 | J = 19.0 ± 0.2 | H = 18.37 ± 0.03 | Ks = 18.9 ± 0.2 | Callanan & Charles (1991); Beekman et al. (1996) | ||
| (QZ Vul) | ||||||||
|
|
||||||||
| GS 1354-64 | R = 20.71 ± 0.03 | Casares et al. (2009) | ||||||
| (BW Cir) | V ~ 21.5 | R ~ 20.5 | i ~ 20.2 | Russell & Lewis (2015) | ||||
|
|
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| H 1705-250 | B + V = 21.5 ± 0.1∗ | R ~ 20.9 ± 0.2 | i′ ~ 20.5 | Martin et al. (1995); Remillard et al. (1996) | ||||
| (N. Oph 77) | Yang et al. (2012) | |||||||
|
|
||||||||
| 3A0620–003 | B = 19.32 ± 0.04 | V = 18.23 ± 0.04 | R = 17.12 ± 0.04 | I = 16.93 ± 0.01 | J = 16.31 ± 0.04 | H = 16.19 ± 0.04 | Cantrell et al. (2010) | |
| V = 18.11 ± 0.01 | I = 17.01 ± 0.04 | J = 16.5 ± 0.1 | H = 16.23 ± 0.02 | Gelino et al. (2001b); Froning & Robinson (2001) | ||||
|
|
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| 1H J1659-487 | r = 19.9 ± 0.1 | Shahbaz et al. (2001) | ||||||
| (GX 339–4) | R = 21.6 ± 0.3 | Lewis et al. (2012) | ||||||
|
|
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| 4U 1543–475 | V ~ 16.6 ± 0.1 | I = 16.1 ± 0.1 | J = 16.04 ± 0.05 | Orosz et al. (1998); Buxton & Bailyn (2004) | ||||
| (IL Lup) | B = 17.3 | V = 16.7 | Chevalier & Ilovaisky (1992) | |||||
Notes. Columns: (1) Name of the dynamical black hole used hereafter; (2–8) quiescent magnitudes reported in different bands; (9) references.
Strictly speaking, Swift J1357.2–0933 is not a dynamical BHTs because it lacks of detection of the secondary star but it has a robust mass function determination.
Since this object has not reached the quiescent level again, the IR magnitudes are values in outburst. The I-band magnitude reported by Boeer et al. (1996) is estimated from a tentative optical counterpart in the field.
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