The Birth of a Relativistic Jet Following the Disruption of a Star by a Cosmological Black Hole
Dheeraj R. Pasham (MIT), Matteo Lucchini (MIT), Tanmoy Laskar,, Benjamin P. Gompertz, Shubham Srivastav, Matt Nicholl, Stephen J. Smartt,, James C. A. Miller-Jones, Kate D. Alexander, Rob Fender, Graham P. Smith,, Michael D. Fulton, Gulab Dewangan, Keith Gendreau

TL;DR
This paper reports multi-wavelength observations of a high-redshift relativistic tidal disruption event, revealing a powerful jet with unique properties that challenge existing jet formation theories.
Contribution
It provides detailed observational evidence and modeling of a relativistic jet from a star disrupted by a supermassive black hole at high redshift, highlighting extreme jet conditions.
Findings
X-ray luminosity exceeds 10^{48} erg/s
Rapid variability on 1000-second timescales
Spectral energy distribution consistent with relativistic jet emission
Abstract
A black hole can launch a powerful relativistic jet after it tidally disrupts a star. If this jet fortuitously aligns with our line of sight, the overall brightness is Doppler boosted by several orders of magnitude. Consequently, such on-axis relativistic tidal disruption events (TDEs) have the potential to unveil cosmological (redshift 1) quiescent black holes and are ideal test beds to understand the radiative mechanisms operating in super-Eddington jets. Here, we present multi-wavelength (X-ray, UV, optical, and radio) observations of the optically discovered transient \target at . Its unusual X-ray properties, including a peak observed luminosity of 10 erg s, systematic variability on timescales as short as 1000 seconds, and overall duration lasting more than 30 days in the rest-frame are traits associated with relativistic TDEs. The X-ray to…
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