aalto1 untyped-item.component.html
JWST Discovery of a High-redshift Tidal Disruption Event Candidate in COSMOS-Web
Loading...
Access rights
openAccess
CC BY
CC BY
Creative Commons license
Except where otherwised noted, this item's license is described as openAccess
publishedVersion
URL
Journal Title
Journal ISSN
Volume Title
A1 Alkuperäisartikkeli tieteellisessä aikakauslehdessä
This publication is imported from Aalto University research portal.
View publication in the Research portal (opens in new window)
View/Open full text file from the Research portal (opens in new window)
View publication in the Research portal (opens in new window)
View/Open full text file from the Research portal (opens in new window)
Unless otherwise stated, all rights belong to the author. You may download, display and print this publication for Your own personal use. Commercial use is prohibited.
Date
Department
Major/Subject
Mcode
Degree programme
Language
en
Pages
19
Series
Astrophysical Journal, Volume 990, issue 2, pp. 1-19
Abstract
The rates and properties of tidal disruption events (TDEs) provide valuable insights into their host galaxy central stellar densities and the demographics of their central supermassive black holes. TDEs have been observed only at low redshifts (z ≲ 1), due to the difficulty in conducting deep time-domain surveys. In this work, we present the discovery of a high-redshift TDE candidate, HZTDE-1, in the COSMOS-Web survey with JWST’s NIRCam, using a novel selection technique based on color and morphology. We outline a methodology for identifying high-z TDEs in deep infrared imaging surveys, leveraging the unique spectral energy distributions and morphologies of these transients. While focused on TDEs, this methodology could also be applied to find other UV-bright transients, such as superluminous supernovae (SLSNe). We apply this technique to COSMOS-Web in filters F115W, F150W, F277W, and F444W, and identify HZTDE-1, a transient point source relative to archival UltraVISTA infrared observations. If we assume it is a TDE, we estimate a photometric redshift of z = 5.0 2 − 1.11 + 1.32 . HZTDE-1 cannot be explained by reasonable supernova or active galactic nuclei models. However, an SLSN at z ≳ 3 can also plausibly explain this transient and would be the highest-redshift SLSN yet known. If confirmed with follow-up observations, HZTDE-1 would represent the highest-redshift TDE discovery to date, and suggest an enhancement of the TDE rate in the high-redshift Universe. Our method, which can be applied to future deep surveys with the JWST and Nancy Grace Roman Space Telescope, offers a pathway to identify TDEs at z > 4 and probe black hole demographics at early cosmic times.
Description
Publisher Copyright: © 2025. The Author(s). Published by the American Astronomical Society.
Keywords
Other note
Citation
Karmen, M, Gezari, S, Lambrides, E, Akins, H B, Norman, C, Casey, C M, Pierel, J, Coulter, D, Rest, A, Fox, O D, Ajay, Y, Allen, N, Drakos, N E, Fujimoto, S, Gomez, S, Gozaliasl, G, Ilbert, O, Kartaltepe, J S, Koekemoer, A M, Lane, Z G, McCracken, H J, Paquereau, L, Rhodes, J, Robertson, B E, Shuntov, M, Siebert, M R, Toft, S, Wevers, T & Zenati, Y 2025, 'JWST Discovery of a High-redshift Tidal Disruption Event Candidate in COSMOS-Web', Astrophysical Journal, vol. 990, no. 2, 149, pp. 1-19. https://doi.org/10.3847/1538-4357/adf216
