Inclination effects on the X-ray emission of Galactic black-hole binaries

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Table 1.

List of outbursts and sources.

Object	Outburst	MJD interval	Total exposure	Number of	Inclination	N_H
	epoch		time (ks)	observations		×10²² cm⁻²
4U 1543–475	2002	52443–52565	275.4	20/112	Low	0.43 (1)
MAXI J1836–194	2011	55804–55896	116.9	69/74	Low	0.3 (7)
Cyg X–1	2003–2004	52693–53182	367.4	147/151	Low	0.54 (3)

GX 339–4	2002	52311–52884	495.6	48/267	Intermediate	0.4 (1)
	2004	53050–53498	565.2	152/328
	2007	53769–54678	572.6	191/347
	2010	54889–55618	326.0	107/317
XTE J1650–500	2002	52159–52447	327.9	47/182	Intermediate	0.7 (1)
Swift J1753.5-0127	2005	53553–53819	188.1	72/73	Intermediate	0.2 (5)
	2007–2011	54226–55894	607.2	275/278

XTE J1550–564	2000	51644–51741	128.7	36/236	High	0.65 (1)
	2001–2004	51938–53163	306.5	69/101
GRO J1655–40	2005	53423–53685	2238.3	68/501	High	0.8 (1)
H 1743–322	2003	52740–53055	668.0	42/194	High	2.4 (1)
	2004	53197–53329	79.1	19/49
	2005	53595–53668	46.4	11/23
	2008a	54746–54789	90.8	18/27
	2008b	54743–54849	68.6	36/38
	2009	54980–55039	93.4	15/51
	2010a	55220–55245	47.8	21/33
	2010b	55418–55470	106.8	25/58
	2011	55664–55735	48.2	19/39

XTE J1752–223	2009	55130–55414	408.2	113/207	Intermediate	0.6 (6)
XTE J1817–330	2006	53768–53950	382.3	20/140	High?	0.15 (1)
GS 1354–645	1997	50774–50840	50.5	7/9	High	3.72 (1)
MAXI J1543-564	2010	55465–55567	154.0	6/100	High	1.4 (2)
Swift J1842.5–1124	2008	54656–54803	83.2	31/49	High	0.4 (8)
XTE J1859+226	1999	51463–51749	356.5	25/127	High	0.34 (1)
XTE J1118+480	2000	51633–51764	138.7	47/50	High	0.01 (1)
	2005	53383–53428	71.7	27/39
MAXI J1659–152	2010	55465–55567	140.9	39/66	High?	0.27 (4)

Notes. The fourth column gives the total exposure time of all the observations analyzed. The fifth column gives the number of observations used in the spectral and timing analysis (blue empty circles in Fig. 1) over the total number (blue empty circles plus black dots in Fig. 1).

References. (1) Dunn et al. (2010); (2) Stiele et al. (2012); (3) Hanke et al. (2009); (4) Jonker et al. (2012) (5) Cadolle Bel et al. (2007); (6) Chun et al. (2013); (7) Russell et al. (2014); (8) Zhao et al. (2016).

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