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Table 5

Compilation of various spectral model parameters used in the literature to fit X-ray spectra of HMXBs, accreting magnetars (HMXB-AM), and classical magnetars (M).

Source Model Γ (α) kTcol/kTbb Type Ref.
keV

4U 1909+07 CompTT 1.2 ± 0.1 HMXB Fürst et al. (2012)
IGR J18214-1318 PL+BBODY HMXB Fornasini et al. (2017)
IGR J11215-5952 PL+BBODY HMXB Sidoli et al. (2017)
LMC X-4 PL+BREMSS+BBODY 0.750 ± 0.005 0.400 ± 0.004 HMXB Beri & Paul (2017)
4U 2206+54 BMC HMXB-AM Reig et al. (2012)
4U 2206+54 PL+BB 0.94 ± 0.03 1.63 ± 0.03 HMXB-AM Reig et al. (2012)
4U 0114+65 BMC 1.8 ± 0.2 HMXB-AM This work
4U 0142+61 PL+BB 3.88(1) 0.41 ± 0.10 M Olausen & Kaspi (2014)
SGR 0501+4516 PL+BB 3.84(6) 0.50(2) M Olausen & Kaspi (2014)
SGR 0526-66 PL+BB 0.44(2) M Olausen & Kaspi (2014)
1E 1048.1-5937 PL+BB 3.14(11) 0.56(1) M Olausen & Kaspi (2014)
1E 1547.0-5408 PL+BB 4.0(2) 0.43(3) M Olausen & Kaspi (2014)
CXOU J164710.2-455216 PL+BB 3.86(22) 0.59(6) M Olausen & Kaspi (2014)
1RXS J170849.0-400910 PL+BB 2.80 ± 0.01 M Olausen & Kaspi (2014)
SGR 1806-20 PL+BB 1.6(1) 0.55(7) M Olausen & Kaspi (2014)
1E 1841-045 PL+BB 1.9(2) 0.45(2) M Olausen & Kaspi (2014)
SGR 1900+14 PL+BB 1.9(1) 0.47(2) M Olausen & Kaspi (2014)
SGR 1935+2154 PL+BB 1.8(5) 0.47(2) M Olausen & Kaspi (2014)
1E 2259+586 PL+BB 3.75(4) 0.37(1) M Olausen & Kaspi (2014)

Notes. The original paper provides a full description of the models.

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