Abstract
Abstract We report the non-detection of dispersed bursts between 4 and 8 GHz from 2.5 hr of observations of FRB 20200120E at 6 GHz using the Robert C. Byrd Green Bank Telescope. Our fluence limits are several times lower than the average burst fluences reported at 600 and 1400 MHz. We conclude that these non-detections are either due to high-frequency bursts being weaker and/or scintillation-induced modulated. It is also likely that our observations were non-concurrent with any activity window of FRB 20200120E.
Highlights
Fast rad io b ursts (FRBs) are millisecond -d uration p ulses of extraga lactic orig in
We report the non-det ection of dispersed bursts between 4 and 8 GHz from 2.5 hr of observations of FRB 20200120E at 6 GHz using the Robert C
Rese arch Notes of the AAS ~ ~ Citation Vishal Gajjaret al 2021 Res. Notes AAS S 166
Summary
Fast rad io b ursts (FRBs) are millisecond -d uration p ulses of extraga lactic orig in.
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