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Table 8.

Model B parameters for V404 Cyg epochs.

Model B: C1 × PHABS1 × SMEDGE × (C2 × BORUS02(RED) + C3 × BORUS02(BLUE) + PHABS2 × CABS × CUTOFFPL
+ C4 × CUTOFFPL + PCFABS × BBODY)

Epoch 1 Epoch 2 Epoch 3 Epoch 4 Epoch 5
PHABS1 × SMEDGE

NH, ism 1022 cm−2 0.83 0.83 0.83 0.83 0.83
E keV 8.67 ± 0.05 8.62 ± 0.04 8.5 ± 0.1
τ 0.30 ± 0.02 0.36 0.16 ± 0.01
σ keV 0.5 0.5 0.5

BORUS02

log NH, tor 24.21 24.00 24.58 ± 0.02 24.703 ± 0.006 24.66 ± 0.01
cos(θtor) >0.78 >0.57 0.55 ± 0.01 0.55 ± 0.01 0.56 ± 0.01
cos(θinc) 0.39 0.39 0.39 0.39 0.39
z 0.042 0.056 0.014 0.014 ± 0.001 0.022 ± 0.002

PHABS2 × CABS × CUTOFFPL

log NH, los 24.36 24.24 23.53 23.58 23.57 ± 0.01
Norm 262 92 3.2 ± 0.5 6.1 14.2
Γ 2.6 2.6 1.92 ± 0.05 2.05 2.50 ± 0.02
Ecut keV 21.8 26.4 94 62 >474

PCFABS × BBODY

log NH, bb 23.782 23.73 ± 0.01
Cov 0.821 0.76
Norm 0.32 ± 0.01 0.44
kT keV 1.120 ± 0.005 0.95 ± 0.01

Constants (a)

C1 1.00 0.99 1.01 1.00 1.00
C2 0.11 0.07 7.7 ± 0.7 15.7 ± 0.8 7.3 ± 0.4
C3 0.05 0.10 2.2 8.1 ± 0.6 3.7 ± 0.4
C4 0 0.034 0.24 0.22 ± 0.02 0.185

Fluxes (10−8 erg s−1 cm−2)

Abs. 1.4 ± 0.3 1.36 ± 0.07 4.2 ± 0.5 7.0 ± 0.6 2.8 ± 0.1
Unabs. 23 ± 6 9.8 ± 0.7 5.0 ± 0.5 8.1 ± 0.5 4.0 ± 0.1
 LOS 90% 74% 33% 25% 50%
 Scattered 2% 2% 59% 70% 40%
 Leaked 2% 8% 5% 10%
 BB 8% 22%

Luminosities (b) and Eddington ratio (c) (3–79 keV)

Abs. 1038 erg s−1 0.09 ± 0.03 0.09 ± 0.02 0.29 ± 0.08 0.48 ± 0.10 0.19 ± 0.03
Unabs. 1038 erg s−1 1.6 ± 0.2 0.67 ± 0.13 0.34 ± 0.08 0.55 ± 0.10 0.28 ± 0.04
L/LEdd 0.14 0.06 0.03 ± 0.01 0.05 ± 0.01 0.02 ± 0.01

Both NuSTAR detectors: (A/B) (A/B) (A/B) (A/B) (A/B)
χ2/d.o.f. 877/619 758/510 451/379 1143/828 945/746
1.42 1.49 1.19 1.38 1.27
Single NuSTAR detector: (A) (B) (A) (B) (B)
χ2/d.o.f. 392/308 297/244 207/189 504/401 448/362
1.27 1.22 1.10 1.26 1.24

Notes. Parameters without errors are kept frozen at the value shown. The dash marks components that are not part of the spectral model in a particular data set.

(a)

c1 is a constant between the FPMA and FPMB allowed to vary.

(b)

The following distance estimates have been used: 2.39 ± 0.14 kpc (Miller-Jones et al. 2009).

(c)

The following mass estimates have been used: 9.0 M (Khargharia et al. 2010).

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