collaborators

6 papers

astro-ph.GA2026

A Meta-Learning Framework for Multitask Reverberation Mapping in Active Galactic Nuclei

Aman N. Raju, Andjelka B. Kovačević, Andjelka B. Kovačević +15

The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) is expected to observe active galactic nuclei (AGN) at sky densities of approximately 1000-4000 per sq. deg, en…

astro-ph.GA2026

The Impact of Supermassive Black Holes on Exoplanet Habitability. I. Spanning the Natural Mass Range

Jourdan Waas, Eric S. Perlman, Manasvi Lingam +5

While the influence of supermassive black hole (SMBH) activity on habitability has garnered attention, the specific effects of active galactic nucleus (AGN) winds, particularly ult…

astro-ph.GA2026

Resolving the Multiphase Outflow, Shock Signatures, and PAHs in the AGN-Starburst Composite ULIRG F10565+2448 with JWST MIRI/MRS

Kylie Yui Dan, Jerome Seebeck, Sylvain Veilleux +9

We present new James Webb Space Telescope Mid-Infrared Instrument (MIRI) Medium-Resolution Spectrometer (MRS) observations of the nearby ultra-luminous infrared galaxy F10565+2448.…

astro-ph.HE2026

Where within the 3C 84 jet are -rays produced?

Georgios F. Paraschos, Ioannis Liodakis, Svetlana Jorstad +49

The location of -ray creation and emission within extra-galactic jets is a matter of active debate. One particularly well-suited source to pinpoint the location is the nearby,…

astro-ph.HE2026

Disc Winds From Accreting Systems in the 2040s

Noel Castro Segura, Virginia Cúneo, Francesco Tombesi +9

What does the temporal evolution of disc winds tell us about accreting systems and the accretion process? Studies of accretion-disc outflows across all mass scales, including accre…

astro-ph.HE2025

Comparing observed properties of winds in low-luminosity active galactic nuclei with theoretical predictions

Fangzheng Shi, Feng Yuan, Francesco Tombesi +1

Theoretical and numerical simulations of black hole hot accretion flows have shown the ubiquitous existence of winds and predicted their properties such as velocity and mass flux.…