Coincident gamma-ray emission in the direction of the active repeater FRB 20240114A

ATel #16594; Yi Xing, Wenfei Yu (Shanghai Astronomical Observatory)
on 19 Apr 2024; 02:56 UT
Credential Certification: Wenfei Yu (wenfei@shao.ac.cn)

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Following the recent reports of the discovery of the repeating FRB 20240114A (ATel #16420) and its extreme radio burst activity (bright bursts - ATel #16432; burst storm - Atel #16505; more than a hundred bright bursts - Atel #16565), we performed a search for gamma-ray emission potentially associated with the central engine activities and the bursting activities of the repeater with Fermi LAT at the precise position reported by the recent burst localization with the EVN (Atel #16542), which followed the MeerKAT's initial burst localization to the 1.5 arcsec level (Atel #16446).

We performed an aperture photometry analysis of the public Fermi LAT data. In the 5-day averaged LAT light curves extracted from photons (> 100 MeV) in a sky region centered at the source with the contaminant angle of the LAT point spread function (circular regions with a typical radius of 5.3 degrees or less, depending on photon energies), we found two episodes of enhanced gamma-ray emission in the direction of the FRB source during MJD 60330 - 60340 (2024 Jan 21 - Jan 30) and MJD 60370 - 60385 (2024 March 1 - March 15), which are coincident with the enhanced bursting activities (Atel #16420, 16430, 16433) and the hyper-active burst storms (burst rate increased to ~ 500 per hour, Atel #16505). The 5-day averaged gamma-ray flux level derived by the aperture photometry analysis during the first episode (a 10 day window) had never been reached in the previous year as seen in the Fermi LAT light curve, suggesting a chance possibility of about 0.02% or better for the occurrence of the first episode alone.

There are known Fermi catalog sources nearby: one source within 1 degree, two other sources within 2 degrees, and even six other sources 4-5 degrees away. Based on a customized selection of photons in the two time windows, we further obtained an estimate of the position of the potential variable source responsible for the flux variation, which is in favor of an association with FRB 20240114A rather than an association with those nearby sources. We also noticed that only a few GeV photons have been detected by Fermi/LAT in the data we analyzed. We encourage further multi-wavelength monitoring of the source and the search for similar signatures of variations on these time scales in addition to radio burst detections.

The Fermi LAT light curves are shown here (http://202.127.29.4/wenfei/ATEL_FRB20240114A_LAT.html).

We thank the Fermi Science Support Center (FSSC) for providing public data timely. The Fermi LAT is a pair conversion telescope designed to cover the energy band from 20 MeV to greater than 300 GeV. It is the product of an international collaboration between NASA and DOE in the U.S. and many scientific institutions across France, Italy, Japan and Sweden.