The AT 2018cow-like fast blue optical transient AT2022tsd showed a large number of few-minute-duration, high-luminosity (~10^43 erg/s) flares. We present an intensive search for such flares from another 18cow-like event, AT2024wpp. We have used the Large Array Survey Telescope (LAST) to observe this transient between 28 and 74 days after the approximate time of zero flux. The target was observed for about 23 hours to a sensitivity that allows one to detect 3x10^42 erg/s flares at S/N>5. No optical flares have been found, suggesting a one-sided 2-sigma confidence upper limit of <0.02 on the flare's duty cycle, and flare rate lower than about 0.11/hr. These limits suggest that not all 18cow-like objects display a high rate of minute-timescale luminous flares. This can be explained either by diversity in the 18cow-like population or by viewing angle effects (e.g., beaming), or rather that the optical depth towards the central emitting region did not fall below unity during the particular search window.
@article{arxiv.2508.18359,
title = {A search for minute-time-scale flares from the transient AT\,2024wpp},
author = {Eran O. Ofek and Lior Ozer and Ruslan Konno and Nimrod Strasman and Ping Chen and Sagi Ben-Ami and David Polishook and Alexander Krassilchtchikov and Simone Garrappa and Erez A. Zimmermann and Enrico Segre and Asaf Horowicz and Avishay Gal-Yam and Yarin M. Shani and Stanislav Fainer and Michael Engel and Yahel Sofer-Rimalt and Anna Y. Q. Ho and Yossi Shvartzvald and Ofer Yaron and Kris Rybicki and Arie Blumenzweig and Sarah Spitzer and Ron Arad},
journal= {arXiv preprint arXiv:2508.18359},
year = {2025}
}