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Nine tidal disruption event candidates in <i>eROSITA</i>-DE DR1 discovered through supersoft X-ray selection

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posted on 2025-09-24, 15:25 authored by RAJ Eyles-Ferris, Rhaana StarlingRhaana Starling, PT O’Brien, Kim PageKim Page, Phil EvansPhil Evans
<p dir="ltr">Tidal disruption events (TDEs) are rare and diverse transients that occur when a star is torn apart by a supermassive black hole and accreted, which can result in a supersoft X-ray thermal transient. Here, we present nine TDE candidates identified in eROSITA-DE Data Release 1 through a novel search for such supersoft sources. We select candidates by comparing the catalogued count rates in several combinations of bands and evaluate the nature of selected sources to produce our sample, among which five are entirely new X-ray TDE candidates. All our candidates’ X-ray spectra are consistent with soft thermal emission and we show them to have faded through additional Swift observations and catalogued data. We investigate publicly available data from ground- and space-based telescopes and find two of our sources have optical counterparts and four sources show flaring in their Near-Earth Object Wide-field Infrared Survey Explorer Reactivation Mission infrared (IR) light curves. The high proportion of our sources with IR flares compared to optically selected TDE samples could suggest a link between supersoft X-ray spectra and IR counterparts. We fit the IR light curves with a model of a spherical dust shell heated by the TDE and find these results to be broadly consistent with those of other TDEs with IR counterparts. Finally, we examine the host galaxies and show them to be similar to the general TDE host population.</p>

History

Author affiliation

College of Science & Engineering Physics & Astronomy

Version

  • VoR (Version of Record)

Published in

Monthly Notices of the Royal Astronomical Society

Volume

542

Issue

2

Pagination

1654 - 1672

Publisher

Oxford University Press (OUP)

issn

0035-8711

eissn

1365-2966

Copyright date

2025

Available date

2025-09-24

Language

en

Deposited by

Dr Rhaana Starling

Deposit date

2025-09-11

Data Access Statement

All data used in this work are available publicly from their respective repositories (see footnotes in text for urls).

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