Characterising Fast X-ray Transients in the Einstein Probe Era through Multiwavelength Follow-up
APA
(2025). Characterising Fast X-ray Transients in the Einstein Probe Era through Multiwavelength Follow-up. SciVideos. https://scivideos.org/index.php/icts-tifr/32994
MLA
Characterising Fast X-ray Transients in the Einstein Probe Era through Multiwavelength Follow-up. SciVideos, Oct. 17, 2025, https://scivideos.org/index.php/icts-tifr/32994
BibTex
@misc{ scivideos_ICTS:32994,
doi = {},
url = {https://scivideos.org/index.php/icts-tifr/32994},
author = {},
keywords = {},
language = {en},
title = {Characterising Fast X-ray Transients in the Einstein Probe Era through Multiwavelength Follow-up},
publisher = {},
year = {2025},
month = {oct},
note = {ICTS:32994 see, \url{https://scivideos.org/index.php/icts-tifr/32994}}
}
Abstract
Fast X-ray transients (FXTs) are singular, short bursts in soft X-rays (~0.3–10 keV) that last from minutes to hours. Their origin remains unclear, and they have been associated with various progenitor mechanisms, including long-duration gamma-ray burst association, the tidal disruption of a white dwarf by an intermediate-mass black hole, a magnetar formed as the aftermath of a binary neutron star merger whose spin-down powers the burst, and a core-collapse supernova shock breakout. The newly launched X-ray survey mission, Einstein Probe (EP), is revolutionising the field by enabling the discovery and prompt follow-up of FXTs, effectively doubling the number of known extragalactic events. In my talk, I will discuss our ongoing search for multiwavelength counterparts — particularly at optical and radio wavelengths — of FXTs discovered by EP, and their role in characterising the nature of these transients.