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physics.ed-ph2025

Analyzing New Planetary Systems at School: Applications of Newton's Law of Universal Gravitation and Kepler's Third Law

Rubén Montecinos, Carla Hernández, Irma Fuentes-Morales +4

As scientific knowledge expands, science education may not always keep pace with the latest advancements in astrophysics. A solid scientific education is crucial for preparing stud…

astro-ph.HE2025

The 2025 outburst of IGR J17511-3057: timing and spectral insights from NICER and NuSTAR

A. Sanna, G. K. Jaisawal, T. E. Strohmayer +13

IGR J17511-3057 was observed in a new outburst phase starting in February 2025 and lasting at least nine days. We investigated the spectral and temporal properties of IGR J17511-30…

cs.LG2025

Signatures to help interpretability of anomalies

Emmanuel Gangler, Emille E. O. Ishida, Matwey V. Kornilov +8

Machine learning is often viewed as a black box when it comes to understanding its output, be it a decision or a score. Automatic anomaly detection is no exception to this rule, an…

astro-ph.SR2025

Dynamical mass of the Serpens intermediate-mass young stellar system EC\,95 with DYNAMO--VLBA

Jazmín Ordóñez-Toro, Sergio A. Dzib, Laurent Loinard +8

We present dynamical mass measurements, obtained from multi-epoch Very Long Baseline Interferometry (VLBI) observations, for the young multiple stellar system EC\,95, located in th…

astro-ph.HE2025

Traces of wobbling accretion disk in X-ray pulsar Her X-1 from observations of the ART-XC telescope of the SRG observatory

V. M. Revnivtsev, K. A. Postnov, S. V. Molkov +5

Long uninterrupted observations of the X-ray binary system Her X-1 were performed with the Mikhail Pavlinsky ART-XC telescope of the Spectrum-Röntgen-Gamma (SRG) X-ray Observatory…

astro-ph.SR2025

VLBA Detections in the Oph-S1 Binary System near Periastron Confirmation of its Orbital Elements and Mass

Jazmín Ordóñez-Toro, Sergio A. Dzib, Laurent Loinard +7

Oph-S1 is the most luminous and massive stellar member of the nearby Ophiuchus star-forming region. Previous Very Long Baseline Array (VLBA) observations have shown it to be an int…