SIMBAD references

The AT 2018cow-like fast blue optical transient AT 2022tsd showed a large number of a few-minute-duration, high-luminosity (∼10⁴³ erg s^–1) flares. We present an intensive search for such flares from another 18cow-like event, AT 2024wpp. We have used the Large Array Survey Telescope to observe this transient between 28 and 74 days after the approximate time of zero flux. The target was observed for about 23 hr to a sensitivity that allows one to detect 3 × 10⁴² erg s^–1 flares at a signal-to-noise ratio ≳ 5. No optical flares have been found, suggesting a one-sided 2σ confidence upper limit of <0.02 on the flare's duty cycle, and flare rate lower than about 0.11 hr^–1. 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 toward the central emitting region did not fall below unity during the particular search window.