Journal
ASTROPHYSICAL JOURNAL LETTERS
Volume 897, Issue 1, Pages -Publisher
IOP Publishing Ltd
DOI: 10.3847/2041-8213/ab9a4a
Keywords
Radio transient sources
Categories
Funding
- Department of Defense (DoD) through the National Defense Science and Engineering Graduate (NDSEG) Fellowship Program
- National Science Foundation (NSF) Graduate Research Fellowship [DGE-1144469]
- NWO Vici fellowship
- Jet Propulsion Laboratory's Spontaneous Concept Research and Technology Development program
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The spectra of repeating fast radio bursts (FRBs) are complex and time-variable, sometimes peaking within the observing band and showing a fractional emission bandwidth of about 10%-30%. These spectral features may provide insight into the emission mechanism of repeating FRBs, or they could possibly be explained by extrinsic propagation effects in the local environment. Broadband observations can better quantify this behavior and help to distinguish between intrinsic and extrinsic effects. We present results from a simultaneous 2.25 and 8.36 GHz observation of the repeating FRB 121102 using the 70 m Deep Space Network radio telescope, DSS-43. During the 5.7 hr continuous observing session, we detected six bursts from FRB 121102, which were visible in the 2.25 GHz frequency band. However, none of these bursts were detected in the 8.36 GHz band, despite the larger bandwidth and greater sensitivity in the higher-frequency band. This effect is not explainable by Galactic scintillation and, along with previous multi-band experiments, clearly demonstrates that apparent burst activity depends strongly on the radio frequency band that is being observed.
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