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20242026
most citedRadio Variability in Recently-Quenched Galaxies: The Impact of TDE or AGN Driven Outflows

1 citations · 1 across the 5 of their papers we have counts for

collaborators

7 papers

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.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

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

Utilizing Maximum Variability to Discern TDE Emission from AGN Flares

Samaresh Mondal, K. Decker French

X-ray emission arising from active galactic nucleus (AGN) activity may potentially mimic the expected emission of tidal disruption events (TDEs). Ongoing and upcoming wide-field X-…

astro-ph.GA20251 cited

Radio Variability in Recently-Quenched Galaxies: The Impact of TDE or AGN Driven Outflows

K. Decker French, Kristina Nyland, Pallavi Patil +7

Outflows and jets launched from the nuclei of galaxies emit radio synchrotron emission that can be used to study the impact of accretion energy on the host galaxy. The decades-long…

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…