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Table 1

Results of spectral analysis of Ser X-1 from previous studies.

Instrument Continuum model Reflection model Line model Line energy (keV) Equivalent width Rin (Rg) Incl (deg) Emissivity index log (ξ) Flux (erg/cm2/s) Reference

ASCA bbody+cutpowerlaw Gaussian 6.6 ± 0.17 81 eV Ref. (1)

RXTE bbody pexrav Gaussian Ref. (2)
BeppoSAX bbody+compTT Gaussian 6.46 275 eV Ref. (2)

XMM-Newton diskbb+compTT laor 6.40 86105 eV 416 4050 210 keV: (3.3-4.2) × 10-9 Ref. (3)

suzaku bbody+diskbb+powerlaw diskline 6.83 132 ± 12 eV 7.7 ± 0.5 26 ± 2 0.5-10 keV: (5.9 ± 0.9) × 10-9a Ref. (4)

suzaku bbody+diskbb+powerlaw diskline 6.97 98 eV 8.0 ± 0.3 24 ± 1 0.525 keV: (1.19 ± 0.01) × 10-8 Ref. (5)
suzaku bbody+diskbb+powerlaw reflionx 6 ± 1 16 ± 1 2.6 ± 0.1 0.525 keV: (1.32  ±  0.08) × 10-8 Ref. (5)
XMM-Newton bbody+diskbb+powerlaw diskline 6.666.97 3850 eV 1426 1332 0.525 keV: (0.6−0.7) × 10-8 Ref. (5)
XMM-Newton bbody+diskbb+powerlaw reflionx 15–107 3–9 2.6–2.8 0.525 keV: (0.6-0.7) × 10-8 Ref (5)

NuSTAR bbody+diskbb+powerlaw kerrdisk 6.97 ± 0.01 91 ± 2 eV 10.6 ± 0.6 18 ± 2 0.540 keV: 1.5 × 10-8 Ref. (6)
NuSTAR bbody+diskbb+powerlaw reflionx 68.3 <10 2.30–2.60 Ref. (6)

Chandra bbody+diskbb+powerlaw diskline 6.97 ± 0.02 149 ± 15 eV 7.7 ± 0.1 24 ± 1 Ref (7)
Chandra bbody+diskbb+powerlaw reflionx 7.1 29 ± 1 2.5 Ref. (7)
Chandra bbody+diskbb+powerlaw xillver 8.4 33 ± 1 2.2 Ref. (7)

suzaku bbody+diskbb+powerlaw Guussian 6.4 192 Ref. (8)
suzaku bbody+diskbb+powerlaw diskline 6.97-0.02 147 8.4 22 ± 1 Ref. (8)
suzaku bbody+diskbb+powerlaw bbrefl 6.7 9 3.05 0.525 keV: (1.1 ± 0.06)  × 10-8 Ref. (8)

Notes.

(a)

Estimated only for the continuum component.

Reference. Ref. (1): Church & Balucińska-Church (2001) – Ref. (2): Oosterbroek et al. (2001) Ref. (3): Bhattacharyya & Strohmayer (2007) Ref. (4): Cackett et al. (2008) Ref. (5): Cackett et al. (2010) Ref. (6): Miller et al. (2013) Ref. (7): Chiang et al. (2016a) Ref. (8): Chiang et al. (2016b).

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