activity
20232026
most citedThe population of tidal disruption events discovered with eROSITA

27 citations · 67 across the 15 of their papers we have counts for

collaborators

16 papers

astro-ph.GA2026

Spatially resolved optical and mid-infrared spectroscopy of SDSS1335+0728: implications for the origin of the Ansky event

P. Sánchez-Sáez, M. Masterson, L. Hernández-García +25

The galaxy SDSS1335+0728 brightened abruptly in December 2019 (the Ansky event) and has since been confirmed as the host of extreme X-ray quasi-periodic eruptions (QPEs) of debated…

astro-ph.HE2026

Persistence of the Millihertz X-ray Quasi-Periodic Oscillation in the Active Galactic Nucleus 1ES 1927+654

Megan Masterson, Erin Kara, William N. Alston +15

1ES 1927+654 is an extreme active galactic nucleus (AGN) that has defied our canonical expectations for how AGN appear across the electromagnetic spectrum and how they vary on shor…

astro-ph.HE2026

Ghosts of eruptions past: Searching for historical Galactic supernovae using variable thermal dust echoes and machine learning

Justin Vega, Kishalay De, Ashish Mahabal +4

The Galactic core-collapse supernova (SN) rate is estimated at per century; however, no optically visible SN has been discovered in the past 400 years. Although recor…

astro-ph.HE2025★ 19 cited

SRG/eROSITA No. 5: Discovery of quasi-periodic eruptions every ~3.7 days from a galaxy at z>0.1

R. Arcodia, P. Baldini, A. Merloni +17

Quasi-periodic eruptions (QPEs) are repeating soft X-ray bursts from the nuclei of galaxies, tantalizingly proposed to be extreme mass ratio inspirals. Here, we report the discover…

astro-ph.HE2025★ 3 cited

A new Bowen Fluorescence Flare and Extreme Coronal Line Emitter discovered by SRG/eROSITA

Pietro Baldini, Arne Rau, Riccardo Arcodia +19

The nuclear transient eRASSt J012026.5-292727 (J012026 hereafter) was discovered in the second SRG/eROSITA all-sky survey (eRASS2). The source appeared more than one order of magni…

astro-ph.HE2025★ 27 cited

The population of tidal disruption events discovered with eROSITA

Iuliia Grotova, Arne Rau, Pietro Baldini +13

This paper presents a systematic study of X-ray-selected canonical tidal disruption events (TDEs) discovered in the western Galactic hemisphere of the first two eROSITA all-sky sur…

astro-ph.HE2025★ 1 cited

Discovery of Quasi-periodic Eruptions in the Tidal Disruption Event and Extreme Coronal Line Emitter AT2022upj: implications for the QPE/TDE fraction and a connection to ECLEs

Joheen Chakraborty, Erin Kara, Riccardo Arcodia +10

Quasi-periodic eruptions (QPEs) are recurring soft X-ray transients emerging from the vicinity of supermassive black holes (SMBHs) in nearby, low-mass galaxy nuclei; about ten QPE…

astro-ph.HE2025

Rapidly varying ionization features in a Quasi-periodic Eruption: a homologous expansion model for the spectroscopic evolution

Joheen Chakraborty, Peter Kosec, Erin Kara +9

Quasi-Periodic Eruptions (QPEs) are recurring bursts of soft X-ray emission from supermassive black holes (SMBHs), which a growing class of models explains via extreme mass-ratio i…

astro-ph.HE2025

Distinguishing Tidal Disruption Events and Changing-look Active Galactic Nuclei via Variation of Mid-infrared Color

Yujun Yao, Jingjing Ye, Luming Sun +3

At present, there is a lack of effective probes to distinguish between mid-infrared (MIR) outbursts induced by tidal disruption events (TDEs) and changing-look active galactic nucl…

astro-ph.HE2025★ 7 cited

eRO-ExTra: eROSITA extragalactic non-AGN X-ray transients and variables in eRASS1 and eRASS2

Iuliia Grotova, Arne Rau, Mara Salvato +19

(Abridged) While previous X-ray studies showed the dominance of regular active galactic nuclei (AGN) variability, a small fraction of sources arise from more exotic phenomena such…

astro-ph.HE2025

Millihertz Oscillations Near the Innermost Orbit of a Supermassive Black Hole

Megan Masterson, Erin Kara, Christos Panagiotou +22

Recent discoveries from time-domain surveys are defying our expectations for how matter accretes onto supermassive black holes (SMBHs). The increased rate of short-timescale, repet…

astro-ph.HE2024

AT 2020nov: Evidence for Disk Reprocessing in a Rare Tidal Disruption Event

Nicholas Earl, K. Decker French, Enrico Ramirez-Ruiz +23

We present a detailed analysis of AT 2020nov, a tidal disruption event (TDE) in the center of its host galaxy, located at a redshift of . AT 2020nov exhibits unique feat…

astro-ph.HE2024★ 1 cited

The Interplay between the Disk and Corona of the Changing-look Active Galactic Nucleus 1ES 1927+654

Ruancun Li, Claudio Ricci, Luis C. Ho +4

Time-domain studies of active galactic nuclei (AGNs) offer a powerful tool for understanding black hole accretion physics. Prior to the optical outburst on 23 December 2017, 1ES 19…

astro-ph.HE2024★ 8 cited

Modeling Multiple X-Ray Reflection in Super-Eddington Winds

Zijian Zhang, Lars Lund Thomsen, Lixin Dai +7

It has been recently discovered that a few super-Eddington sources undergoing black hole super-Eddington accretion exhibit X-ray reflection signatures. In such new systems, one exp…

astro-ph.HE2023

The High Energy X-ray Probe (HEX-P): Sensitive broadband X-ray observations of transient phenomena in the 2030s

Murray Brightman, Raffaella Margutti, Ava Polzin +13

HEX-P will launch at a time when the sky is being routinely scanned for transient gravitational wave, electromagnetic and neutrino phenomena that will require the capabilities of a…

astro-ph.HE2023★ 1 cited

The High Energy X-ray Probe (HEX-P): Probing the physics of the X-ray corona in active galactic nuclei

E. Kammoun, A. M. Lohfink, M. Masterson +28

The hard X-ray emission in active galactic nuclei (AGN) and black hole X-ray binaries is thought to be produced by a hot cloud of electrons referred to as the corona. This emission…