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Table C.1.

Best-fit parameters obtained by fitting a standard Kerr mock spectrum (a* = 0.998, i = 75°) using the customized wormhole reflection model (kwconv) and the modular Kerr model (kerrconv).

Component Parameter Unit kwconv (Wormhole) kerrconv (Kerr)
Relativistic a* 0.99985 ± 0.00345 0.99800 ± 0.00651
Convolution θobs deg 75.08 ± 3.97 75.15 ± 0.21
qin 3.90 ± 0.11 3.70 ± 0.08
qout 3.90 (=qin) 10.00 ± 115.7
rbr rg 31.89 ± 3.32 8.10 ± 10.38
rin rg 1.230 ± 0.066 1.00 ± 0.08
rout rg 27.59 ± 1.84 399.8 ± fix
λ 0.0

xillverCp Γ 1.994 ± 0.004 1.998 ± 0.004
AFe 1.001 ± 0.009 0.982 ± 0.008
log ξ 3.114 ± 0.007 3.110 ± 0.008
kTe keV 196.89 ± 15.50 237.71 ± 25.79
log N 15.99 ± 0.03 16.00 ± 0.03
norm 10−5 2.60 ± 0.40 0.38 ± 0.05

Statistics χ2/d.o.f. 1999.65/1884 ≈ 1.061 1955.68/1885 ≈ 1.037
Null hyp. prob. 3.16 × 10−2 0.126

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