Evidence for different accretion regimes in GRO J1008−57

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Table 1

Observations used in this work.

Sat.^a	ObsID	Start (MJD)	Expt.^b	E ^c

Suzaku	907006010	56 251.63	9061	1a
NuSTAR	80001001002	56 261.36	14767	1b
Swift	00031030018	56 261.53	1716	1b
Suzaku	408044010	56 660.66	15322	2
NuSTAR	90001003002	56 994.82	26861	3
Swift	00081425001	56 995.00	2263	3
NuSTAR	90001003004	57 049.74	17260	4
Swift	00081425002	57 049.79	1943	4

Notes. Data from epoch 1a has been used and analyzed by Yamamoto et al. (2013, 2014) as well as by Bellm et al. (2014), who used and analyzed epoch 1b in addition.

^(a)

Name of the X-ray mission.

^(b)

Exposure time in seconds. For NuSTAR the longest FPM and for Suzaku the longest XIS exposure is given.

^(c)

Data epoch indicating which observations have been combined in the spectral analysis.

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