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Cited article:

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An investigation of the ‘10 keV feature’ in the spectra of accretion powered X-ray pulsars with NuSTAR

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Monitoring observations of SMC X-1’s excursions (MOOSE)–I. Programme description and initial high state spectral results

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Is Superorbital Modulation in SMC X-1 Caused by Absorption in a Warped Precessing Accretion Disk?

Pragati Pradhan, Chandreyee Maitra and Biswajit Paul
The Astrophysical Journal 895 (1) 10 (2020)
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Observing the Transient Pulsations of SMC X-1 with NuSTAR

Sean N. Pike, Fiona A. Harrison, Matteo Bachetti, McKinley C. Brumback, Felix S. Fürst, Kristin K. Madsen, Katja Pottschmidt, John A. Tomsick and Jörn Wilms
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A new possible accretion scenario for ultra-luminous X-ray sources

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X-Ray Reprocessing: Through the Eclipse Spectra of High-mass X-Ray Binaries with XMM-Newton

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X-ray detection of warm ionized matter in the Galactic halo

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A thin diffuse component of the Galactic ridge X-ray emission and heating of the interstellar medium contributed by the radiation of Galactic X-ray binaries

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POSSIBLE DETECTION OF A CYCLOTRON RESONANCE SCATTERING FEATURE IN THE X-RAY PULSAR 4U 1909+07

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X-RAY SPECTROSCOPY OF THE HIGH-MASS X-RAY BINARY PULSAR CENTAURUS X-3 OVER ITS BINARY ORBIT

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The Astrophysical Journal 737 (2) 79 (2011)
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Suzaku observation of the transient X-ray pulsar GRO J1008−57

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Broadband X‐Ray Spectroscopy of A0535+262 withSuzaku

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Probing the nature of IGR J16493−4348: spectral and temporal analysis of the 1-100 keV emission

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Quasi‐periodic Oscillations in XTE J0111.2−7317: Highest Frequency among the HMXB Pulsars

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The Astrophysical Journal 660 (2) 1409 (2007)
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Discovery of the Millisecond X‐Ray Pulsar HETE J1900.1−2455

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Broadband X‐Ray Spectrum of KS 1947+300 withBeppoSAX

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Photoionized Lines in X‐Ray Spectra of SMC X‐1

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Pulse‐Phase Spectroscopy of SMC X‐1 withChandraandXMM‐Newton: Reprocessing by a Precessing Disk?

R. C. Hickox and S. D. Vrtilek
The Astrophysical Journal 633 (2) 1064 (2005)
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Phase Variation in the Pulse Profile of SMC X-1

J. Neilsen, R. C. Hickox and S. D. Vrtilek
The Astrophysical Journal 616 (2) L135 (2004)
https://doi.org/10.1086/426890