Simultaneous X-Ray and Radio Observations of the Repeating Fast Radio Burst FRB similar to 180916.J0158+65
Artikel i vetenskaplig tidskrift, 2020
We report on simultaneous radio and X-ray observations of the repeating fast radio burst source FRB 180916.J0158+65 using the Canadian Hydrogen Intensity Mapping Experiment (CHIME), Effelsberg, and Deep Space Network (DSS-14 and DSS-63) radio telescopes and the Chandra X-ray Observatory. During 33 ks of Chandra observations, we detect no radio bursts in overlapping Effelsberg or Deep Space Network observations and a single burst during CHIME/FRB source transits. We detect no X-ray events in excess of the background during the Chandra observations. These non-detections imply a 5 sigma limit of <5 x 10(-10)erg cm(-2)for the 0.5-10 keV fluence of prompt emission at the time of the radio burst and 1.3 x 10(-9)erg cm(-2)at any time during the Chandra observations. Given the host-galaxy redshift of FRB 180916.J0158+65 (z similar to 0.034), these correspond to energy limits of <1.6 x 10(45)erg and <4 x 10(45)erg, respectively. We also place a 5 sigma limit of <8 x 10(-15)erg s(-1) cm(-2)on the 0.5-10 keV absorbed flux of a persistent source at the location of FRB 180916.J0158+65. This corresponds to a luminosity limit of <2 x 10(40)erg s(-1). Using an archival set of radio bursts from FRB 180916.J0158+65, we search for prompt gamma-ray emission in Fermi/GBM data but find no significant gamma-ray bursts, thereby placing a limit of 9 x 10(-9)erg cm(-2)on the 10-100 keV fluence. We also search Fermi/LAT data for periodic modulation of the gamma-ray brightness at the 16.35 days period of radio burst activity and detect no significant modulation. We compare these deep limits to the predictions of various fast radio burst models, but conclude that similar X-ray constraints on a closer fast radio burst source would be needed to strongly constrain theory.
X-ray bursts
Radio transient sources
High energy astrophysics
Neutron stars
Författare
P. Scholz
University of Toronto
A. Cook
University of Toronto
M. Cruces
Max-Planck-Gesellschaft
J. W. T. Hessels
Universiteit Van Amsterdam
Netherlands Institute for Radio Astronomy (ASTRON)
V. M. Kaspi
McGill University
W. A. Majid
California Institute of Technology (Caltech)
A. Naidu
McGill University
A. B. Pearlman
California Institute of Technology (Caltech)
L. G. Spitler
Max-Planck-Gesellschaft
K. M. Bandura
West Virginia University
M. Bhardwaj
McGill University
T. Cassanelli
University of Toronto
P. Chawla
McGill University
B. M. Gaensler
University of Toronto
D. C. Good
University of British Columbia (UBC)
A. Josephy
McGill University
R. Karuppusamy
Max-Planck-Gesellschaft
A. Keimpema
Joint Institute for VLBI in Europe (JIVE)
A. Yu Kirichenko
Russian Academy of Sciences
Universidad Nacional Autónoma de México
Franz Kirsten
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
J. Kocz
California Institute of Technology (Caltech)
C. Leung
Massachusetts Institute of Technology (MIT)
B. Marcote
Joint Institute for VLBI in Europe (JIVE)
K. Masui
Massachusetts Institute of Technology (MIT)
J. Mena-Parra
Massachusetts Institute of Technology (MIT)
M. Merryfield
McGill University
D. Michilli
McGill University
C. J. Naudet
California Institute of Technology (Caltech)
K. Nimmo
Universiteit Van Amsterdam
Netherlands Institute for Radio Astronomy (ASTRON)
Z. Pleunis
McGill University
T. A. Prince
California Institute of Technology (Caltech)
M. Rafiei-Ravandi
Perimeter Institute for Theoretical Physics
M. Rahman
University of Toronto
K. Shin
Massachusetts Institute of Technology (MIT)
K. M. Smith
Perimeter Institute for Theoretical Physics
I. H. Stairs
University of British Columbia (UBC)
S. P. Tendulkar
McGill University
K. Vanderlinde
University of Toronto
Astrophysical Journal
0004-637X (ISSN) 1538-4357 (eISSN)
Vol. 901 2 165Ämneskategorier
Subatomär fysik
Astronomi, astrofysik och kosmologi
Annan fysik
DOI
10.3847/1538-4357/abb1a8