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  5. Gamma-Ray and X-Ray Observations of the Periodic-repeater FRB 180916 during Active Phases
 

Gamma-Ray and X-Ray Observations of the Periodic-repeater FRB 180916 during Active Phases

Journal
THE ASTROPHYSICAL JOURNAL LETTERS  
Date Issued
2020
Author(s)
TAVANI, MARCO  
•
VERRECCHIA, Francesco  
•
CASENTINI, CLAUDIO  
•
PERRI, Matteo  
•
URSI, ALESSANDRO  
•
PACCIANI, LUIGI  
•
PITTORI, Carlotta  
•
BULGARELLI, ANDREA  
•
PIANO, Giovanni  
•
PILIA, Maura  
•
BERNARDI, GIANNI  
•
Addis, A.
•
ANTONELLI, Lucio Angelo  
•
ARGAN, ANDREA  
•
Baroncelli, L.  
•
CARAVEO, PATRIZIA  
•
Cattaneo, P. W.
•
Chen, A.
•
Costa, E.  
•
DI PERSIO, GIUSEPPE  
•
Donnarumma, I.
•
EVANGELISTA, YURI  
•
FEROCI, MARCO  
•
Ferrari, A.
•
FIORETTI, VALENTINA  
•
LAZZAROTTO, FRANCESCO  
•
Longo, F.
•
Morselli, A.
•
Paoletti, F.
•
PARMIGGIANI, NICOLO  
•
TROIS, ALESSIO  
•
VERCELLONE, STEFANO  
•
NALDI, Giovanni  
•
PUPILLO, Giuseppe  
•
BIANCHI, GERMANO  
•
Puccetti, S.
DOI
10.3847/2041-8213/ab86b1
Abstract
FRB 180916 is a most intriguing source capable of producing repeating fast radio bursts with a periodic 16.3 day temporal pattern. The source is well positioned in a star-forming region in the outskirts of a nearby galaxy at 150 Mpc distance. In this Letter we report on the X-ray and γ-ray observations of FRB 180916 obtained by AGILE and Swift. We focused especially on the recurrent 5 day time intervals of enhanced radio bursting. In particular, we report on the results obtained in the time intervals 2020 February 3-8, 2020 February 25, 2020 March 5-10, and 2020 March 22-28 during a multiwavelength campaign involving high-energy and radio observations of FRB 180916. We also searched for temporal coincidences at millisecond timescales between the 32 known radio bursts of FRB 180916 and X-ray and MeV events detectable by AGILE. We do not detect any simultaneous event or any extended X-ray and γ-ray emission on timescales of hours/days/weeks. Our cumulative X-ray (0.3-10 keV) flux upper limit of 5 × 10-14 erg cm-2 s-1 (obtained during 5 day active intervals from several 1-2 ks integrations) translates into an isotropic luminosity upper limit of LX,UL ∼ 1.5 × 1041 erg s-1. Deep γ-ray observations above 100 MeV over a many-year timescale provide an average luminosity upper limit one order of magnitude larger. These results provide the so-far most stringent upper limits on high-energy emission from the FRB 180916 source. Our results constrain the dissipation of magnetic energy from a magnetar-like source of radius Rm, internal magnetic field Bm, and dissipation timescale τd to satisfy the relation ${R}_{m,6}^{3}\,{B}_{m,16}^{2}\,{\tau }_{d,8}^{-1}\lesssim 1$ , where Rm,6 is Rm in units of 106 cm, Bm,16 is Bm in units of 1016 G, and τd,8 in units of 108 s.
Volume
893
Issue
2
Start page
L42
Uri
http://hdl.handle.net/20.500.12386/32017
Url
https://api.elsevier.com/content/abstract/scopus_id/85085117164
https://iopscience.iop.org/article/10.3847/2041-8213/ab86b1
Issn Identifier
2041-8205
Ads BibCode
2020ApJ...893L..42T
Rights
open.access
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