24–28 Mar 2025
Florence, Italy
Europe/Rome timezone

Swift's crucial role in the Einstein Probe era of Fast X-ray Transients

27 Mar 2025, 10:15
15m
Florence, Italy

Florence, Italy

Piazza Adua, 1, 50123 Firenze, Italia

Speaker

Peter Jonker

Description

Fast X-ray Transients (FXTs) are minute-to-hours long flashes of
X-rays, first discovered serendipitously in X-ray satellite data
(e.g., Chandra, XMM-Newton, and Swift). They are proven to be caused by
energetic extra-galactic phenomena. Currently, Einstein Probe is
revolutionizing the field by discovering many FXTs and, crucially, by
their low-latency announcement thereof. These extra-galactic FXTs are
ubiquitous: their density rate is several hundred per year per
Mpc^3. FXTs have been proposed to arise from double neutron star
mergers, tidal disruption events involving an intermediate-mass black
hole and a white dwarf, and from off-axis or sub-luminous gamma-ray
bursts. Brief extra-galactic FXTs also arise in supernova shock
breakouts. Contemporaneous multi-wavelength detections possible only
in the current Einstein Probe era show that FXTs originate from more
than 1 progenitor. Swift's (autonomous, level 0) follow-up of Einstein Probe-discovered events provides crucial rapid accurate localizations (XRT/UVOT) and early UVOT multi-wavelength information. We will discuss the most recent findings and provide some (potential) science questions to be answered using FXT observations.

Primary author

Co-authors

Prof. Andrew Levan (Radboud University) Dr Daniele Malesani (Dark) Dr Jonathan Quirola-Vásquez (Radboud University)

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