collaborators

6 papers

astro-ph.HE2026

X-ray luminous late-type giants: an overlooked population contributing to the Galactic ridge iron line emission

Tong Bao, Gabriele Ponti, Xiao-jie Xu +8

The origin of the highly ionized iron emission (Fe XXV at ) characterizing the Galactic ridge X-ray emission (GRXE) remains a fundamental puzzle in high-energy a…

astro-ph.HE2026

STONKS first results: Long-term transients in the XMM-Newton Galactic plane survey

Robbie Webbe, E. Quintin, N. A. Webb +5

The study of astronomical transients at high energies provides insights into some of the most extreme physical events in the universe; however, carrying out their detection and fas…

astro-ph.HE2026

The Advanced X-ray Imaging Satellite (AXIS) Community Science Book

Michael Koss, Nafisa Aftab, Steven W. Allen +395

The AXIS Community Science Book represents the collective effort of 592 scientists worldwide to define the transformative science enabled by the Advanced X-ray Imaging Satellite (A…

astro-ph.HE2025

The very faint X-ray transient Swift J174610-290018 at the Galactic center

Giovanni Stel, Gabriele Ponti, Nathalie Degenaar +17

Very Faint X-ray Transients (VFXTs) are a class of X-ray binary systems that exhibit occasional outbursts with peak X-ray luminosities (L_X< 1e36 erg s^-1) much lower than typical…

astro-ph.HE2025

Unveiling the soft X-ray source population towards the inner Galactic disk with XMM-Newton

Tong Bao, Gabriele Ponti, Frank Haberl +5

Across the Galactic disk lies a diverse population of X-ray sources, with the fainter end remaining poorly understood due to past survey sensitivity limits. We aim to classify and…

astro-ph.HE2025

A sample of ionised Fe line-emitting X-ray sources in the inner Galactic disc

Samaresh Mondal, Gabriele Ponti, Tong Bao +4

Previous studies suggest that the Galactic diffuse X-ray emission is composed of unresolved point sources, primarily mCVs. However, nearby mCVs have a much lower 6.7 keV line equiv…