Constraints on the X-ray-to-radio fluence ratio of FRB 20240114A
arXiv:2503.02580 · doi:10.1051/0004-6361/202453563
Abstract
We report on multiwavelength observations of FRB 20240114A, a nearby (z=0.13), hyperactive, repeating fast radio burst that was discovered in January 2024. We performed simultaneous observations of the source with the Effelsberg 100-m radio telescope, the Thai National Radio Telescope, the Astropeiler Stockert, and the X-ray satellite XMM-Newton in May 2024. On May 23, 2024, we detected 459 bursts from the source using the Ultra-Broad-Band (UBB) receiver of the Effelsberg telescope, covering a frequency range from 1.3 GHz to 6 GHz. All bursts have simultaneous X-ray coverage, which allows us to put stringent constraints on the X-ray-to-radio fluence ratio, , of FRB 20240114A. In this work, we focus on the three brightest radio bursts detected during the campaign. The brightest burst exhibits a radio fluence of erg cm, while the upper limit of the 0.212 keV absorption-corrected X-ray burst fluence lies in the range of erg cm to erg cm, depending on the spectral model. Assuming a 10 keV black-body spectrum, the X-ray-to-radio fluence ratio can be constrained to . A cutoff power law (, cutoff at 84 keV) is also considered, physically motivated by the Galactic magnetar SGR 1935+2154, which has previously shown X-ray bursts associated with FRB-like radio bursts at a measured X-ray-to-radio fluence ratio of (1250 keV). In this scenario, we find that . Our results are consistent with FRB 20240114A being powered by a mechanism similar to that of SGR 1935+2154. We show that future multiwavelength campaigns will be able to improve this limit if sufficiently bright radio bursts are observed with simultaneous X-ray coverage.
arXiv comment6 pages, 2 figures, 2 tables, accepted for publication in A&A
References in corpus (30)
- Gaia Data Release 3: Summary of the content and survey properties
- HI4PI: A full-sky HI survey based on EBHIS and GASS
- A fast radio burst associated with a Galactic magnetar
- DSPSR: Digital Signal Processing Software for Pulsar Astronomy
- A Living Theory Catalogue for Fast Radio Bursts
- Fast radio bursts as synchrotron maser emission from decelerating relativistic blast waves
- An Accurate Flux Density Scale from 50 MHz to 50 GHz
- INTEGRAL discovery of a burst with associated radio emission from the magnetar SGR 1935+2154
- The repeating Fast Radio Burst FRB 121102: Multi-wavelength observations and additional bursts
- FRB 121102 Bursts Show Complex Time-Frequency Structure
- HXMT Identification of a non-thermal X-ray burst from SGR J1935+2154 and with FRB 200428
- A peculiar hard X-ray counterpart of a Galactic fast radio burst
- PINT: A Modern Software Package for Pulsar Timing
- FRB Energetics and detectability from high redshifts
- Implications of a "Fast Radio Burst" from a Galactic Magnetar
- FETCH: A deep-learning based classifier for fast transient classification
- The Northern High Time Resolution Universe Pulsar Survey I: Setup and initial discoveries
- Simultaneous X-ray, gamma-ray, and Radio Observations of the repeating Fast Radio Burst FRB 121102
- The lowest frequency Fast Radio Bursts: Sardinia Radio Telescope detection of the periodic FRB 180916 at 328 MHz
- The High Time Resolution Universe survey XIV: Discovery of 23 pulsars through GPU-accelerated reprocessing
- A radio pulsar phase from SGR J1935+2154 provides clues to the magnetar FRB mechanism
- Simultaneous X-ray and Radio Observations of the Repeating Fast Radio Burst FRB 180916.J0158+65
- The Fast Radio Burst FRB 20201124A in a star forming region: constraints to the progenitor and multiwavelength counterparts
- NuSTAR observations of X-ray bursts from the magnetar 1E 1048.1-5937
- Multiwavelength Constraints on the Origin of a Nearby Repeating Fast Radio Burst Source in a Globular Cluster
- The new magnetar SGR J1830-0645 in outburst
- Multimoment Radio Transient Detection
- Simultaneous and panchromatic observations of the Fast Radio Burst FRB 20180916B
- Contemporaneous X-ray Observations of 30 Bright Radio Bursts from the Prolific Fast Radio Burst Source FRB 20220912A
- Symmetry Breaking in Repeating Fast Radio Bursts