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Cited article:

Discovery of a New Phase-transient Cyclotron Line in A0535+26: Constraints on the Accretion Geometry

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The Astrophysical Journal 981 (2) 205 (2025)
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Cyclotron line evolution revealed with pulse-to-pulse analysis in the 2020 outburst of 1A 0535+262

Qing C Shui, S Zhang, Peng J Wang, Alexander A Mushtukov, A Santangelo, Shuang N Zhang, Ling D Kong, L Ji, Yu P Chen, V Doroshenko, F Frontera, Z Chang, Jing Q Peng, Hong X Yin, Jin L Qu, L Tao, Ming Y Ge, J Li, Wen T Ye and Pan P Li
Monthly Notices of the Royal Astronomical Society 528 (4) 7320 (2024)
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A polarimetrically oriented X-ray stare at the accreting pulsar EXO 2030+375

Christian Malacaria, Jeremy Heyl, Victor Doroshenko, Sergey S. Tsygankov, Juri Poutanen, Sofia V. Forsblom, Fiamma Capitanio, Alessandro Di Marco, Yujia Du, Lorenzo Ducci, Fabio La Monaca, Alexander A. Lutovinov, Herman L. Marshall, Ilya A. Mereminskiy, Sergey V. Molkov, Alexander A. Mushtukov, Mason Ng, Pierre-Olivier Petrucci, Andrea Santangelo, Andrey E. Shtykovsky, Valery F. Suleimanov, Iván Agudo, Lucio A. Antonelli, Matteo Bachetti, Luca Baldini, et al.
Astronomy & Astrophysics 675 A29 (2023)
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Supercritical accretion of BeXRB SXP 15.3

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Monthly Notices of the Royal Astronomical Society 520 (3) 3396 (2023)
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Study of timing and spectral properties of the X-ray pulsar 1A 0535+262 during the giant outburst in 2020 November–December

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Monthly Notices of the Royal Astronomical Society 511 (1) 1121 (2022)
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Variations in energy of cyclotron lines with double structures formed in a line-forming region with bulk motion in accreting X-ray pulsars

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Publications of the Astronomical Society of Japan 74 (4) 961 (2022)
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Comprehensive broad-band study of accreting neutron stars with Suzaku: Is there a bi-modality in the X-ray spectrum?

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The Ups and Downs of Accreting X-Ray Pulsars: Decade-long Observations with the Fermi Gamma-Ray Burst Monitor

C. Malacaria, P. Jenke, O. J. Roberts, C. A. Wilson-Hodge, W. H. Cleveland and B. Mailyan
The Astrophysical Journal 896 (1) 90 (2020)
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The First NuSTAR Observation of 4U 1538–522: Updated Orbital Ephemeris and a Strengthened Case for an Evolving Cyclotron Line Energy

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NICER and Fermi GBM Observations of the First Galactic Ultraluminous X-Ray Pulsar Swift J0243.6+6124

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Luminosity-dependent changes of the cyclotron line energy and spectral hardness in Cepheus X-4

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Astronomy & Astrophysics 601 A126 (2017)
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The Strongest Magnetic Fields in the Universe

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Evidence for an evolving cyclotron line energy in 4U 1538−522

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Monthly Notices of the Royal Astronomical Society 458 (3) 2745 (2016)
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THE TRANSIENT ACCRETING X-RAY PULSAR XTE J1946+274: STABILITY OF X-RAY PROPERTIES AT LOW FLUX AND UPDATED ORBITAL SOLUTION

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The Astrophysical Journal 815 (1) 44 (2015)
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Luminosity-dependent spectral and timing properties of the accreting pulsar GX 304−1 measured with INTEGRAL

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