Luminous Fast Blue Optical Transients (LFBOTs) are a class of extragalactic transient of uncertain origin. Several hypotheses have been put forward which could feasibly be consistent with the sample number of events discovered thus far, including tidal disruption events around intermediate mass black holes, failed supernovae and mergers of stars with black holes. Whatever their origin, it is clear that better understanding LFBOTs will provide unique insight into the black hole formation/growth, central engine physics and transient-host galaxy interactions - themes which are expected to drive research in transient astronomy over the coming decades. The vast majority of LFBOTs are missed by current photometric surveys, or not efficiently selected for detailed follow-up. This white paper outlines the observing capabilities required on a 2040 timescale to maximise the discovery potential from these enigmatic events.
Cite
@article{arxiv.2512.14832,
title = {Luminous Fast Blue Optical Transients in the 2040s},
author = {A. A. Chrimes and N. Sarin and D. Coppejans and P. J. Groot and A. Inkenhaag and P. G. Jonker and T. L. Killestein and D. A. Perley and M. Pursiainen},
journal= {arXiv preprint arXiv:2512.14832},
year = {2025}
}
Comments
White paper submitted for the ESO Expanding Horizons initiative