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Cited article:

Is There a Retrograde Accretion Disk around 4U 1626–67? Tracking Torque Reversals with a State-space Model

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The Astrophysical Journal 997 (1) 130 (2026)
https://doi.org/10.3847/1538-4357/ae2610

Double-hump spectrum, pulse profile dip, and pulsed fraction spectra from the low-accretion regime in the X-ray pulsar MAXI J0655-013

C. Malacaria, S. N. Pike, A. D’Aì, G. L. Israel, L. Ducci, R. E. Rothschild, L. Stella, R. Amato, E. Ambrosi, J. B. Coley, F. Fürst, M. Imbrogno, P. Kretschmar, D. K. Maniadakis, A. Papitto, P. Pradhan, A. Rouco Escorial, A. Simongini, J. Stierhof, B. F. West and N. Zalot
Astronomy & Astrophysics 706 A321 (2026)
https://doi.org/10.1051/0004-6361/202557862

The elusive cyclotron line in 4U 1901+03: Hidden, yet present

Elena Ambrosi, Antonino D’Aí, Giancarlo Cusumano, Carlo Ferrigno, Ekaterina Sokolova-Lapa, Dimitrios K. Maniadakis, Antonio Tutone, Georgios Vasilopoulos, Peter Kretschmar, Christian Malacaria and Fabio Pintore
Astronomy & Astrophysics 709 A42 (2026)
https://doi.org/10.1051/0004-6361/202557808

Magellanic Accretion-powered Pulsars Studied via an Unscented Kalman Filter

Dimitris M. Christodoulou, Joseph O’Leary, Andrew Melatos, Tom Kimpson, Sayantan Bhattacharya, Nicholas J. O’Neill, Silas G. T. Laycock and Demosthenes Kazanas
The Astrophysical Journal 988 (2) 275 (2025)
https://doi.org/10.3847/1538-4357/ade87b