The X-ray view of black-hole candidate Swift J1842.5-1124 during its 2008 outburst

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Table 1

Best fit results for Swift/XRT observations.

Obs. ID	MJD	N_H	kT	Γ	Flux_Po	Flux_Total	χ²/d.o.f.
		(10²² cm^-2)	(keV)		(10^-9 erg cm^-2 s^-1)	(10^-9 erg cm^-2 s^-1)

00031234001^§	54 654.6		–				25.0/36
00031234002	54 656.6						217.6/249
00031234003^§	54 657.3		–				14.9/19
00031234004^§	54 658.3		–				42.2/41
00031234005^§	54 659.9		–				48.7/52
00031234006^§	54 660.4		–				77.4/74
00324112000^♯	54 717.3						198.0/187
00031234007	54 720.8						355.6/301
00031234008	54 721.7						434.0/398
00031234009	54 722.5						321.5/324
00031234010	54 730.6						597.1/552
00031234011	54 751.1						760.4/525
00031234012	54 752.8						574.5/496
00031234013	54 765.9						531.1/543
00031234014	54 779.2						497.4/418

Notes. Flux_Po: 0.6–10 keV unabsorbed flux for the power-law component. Flux_Total: total unabsorbed flux calculated in 0.6–10 keV.

^(§)

Observations were operated in the photon-counting mode, and the rest of Swift/XRT observations were executed in the window-timing mode.

^(♯)

There were two short automated observations (Obs IDs = 00324112000 and 00324116000) performed within two hours on 2008 September 14 (MJD = 54 717); hence we fit them together in order to improve the signal-to-noise.

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