A Target Search for Fast Radio Bursts Associated with Two Fast Blue Optical Transients: AT2018cow and CSS161010
Shi-Jie Gao, Xiang-Dong Li, Yi-Xuan Shao, Ping Zhou, Pei Wang, Yun-Wei Yu, Zhen Yan, Di Li

TL;DR
This study conducted deep radio observations of two FBOTs to search for associated FRBs, setting upper limits on their radio transient emissions and constraining the activity of potential magnetar sources.
Contribution
It provides the most stringent upper limits on FRB-like signals from FBOTs and constrains the burst rate from potential magnetars within these events.
Findings
No FRB-like signals detected from the two FBOTs.
Constraints on the burst rate from potential magnetars in FBOTs.
Implication that FRB activity, if present, is weaker or less frequent than in known FRB sources.
Abstract
Fast blue optical transients (FBOTs) are luminous, rapidly evolving events with blue spectra, possibly powered by newborn magnetars and linked to fast radio bursts (FRBs). Given this potential connection, we conducted deep radio observations of two nearby FBOTs (AT2018cow and CSS161010) using the Five-hundred-meter Aperture Spherical radio Telescope (FAST), but detected no FRB-like signals. Our observations establish the most stringent upper limits on millisecond radio transients from FBOTs, reaching 10 mJy flux density. Assuming a log-normal luminosity function analogous to the repeating FRB 121102, we constrain the burst rate from potential magnetars in FBOTs to hr. The short ejecta escape timescale (2.6 yr) compared to our observation epochs (46 years post-explosion) suggests that nondetection may not be attributed to FBOT's ejecta absorption. These…
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