scholarly journals Statistical properties of the repeating fast radio burst source FRB 121102

2019 ◽  
Vol 1 (1) ◽  
pp. 22-32 ◽  
Author(s):  
Bing Li ◽  
Long-Biao Li ◽  
Zhi-Bin Zhang ◽  
Jin-Jun Geng ◽  
Li-Ming Song ◽  
...  
Keyword(s):  
Radio Burst ◽  
Statistical Properties ◽  
Burst Source ◽  
Fast Radio Burst

scholarly journals A repeating fast radio burst source localized to a nearby spiral galaxy

Nature ◽  
2020 ◽  
Vol 577 (7789) ◽  
pp. 190-194 ◽  
Author(s):  
B. Marcote ◽  
K. Nimmo ◽  
J. W. T. Hessels ◽  
S. P. Tendulkar ◽  
C. G. Bassa ◽  
...  
Keyword(s):  
Spiral Galaxy ◽  
Radio Burst ◽  
Burst Source ◽  
Fast Radio Burst

scholarly journals Scale-invariance in the repeating fast radio burst 121102

2019 ◽  
Author(s):  
Hai-Nan Lin ◽  
Yu Sang
Keyword(s):  
Total Energy ◽  
Flux Density ◽  
Radio Burst ◽  
Probability Density Functions ◽  
Statistical Properties ◽  
Density Functions ◽  
Scale Invariant ◽  
Invariant Structure ◽  
Fast Radio Burst ◽  
Soft Gamma Repeater

Abstract The statistical properties of the repeating fast radio burst FRB 121102 are investigated. We find that the cumulative distributions of fluence, flux density, total energy and waiting time can be well fitted by the bent power law. In addition, the probability density functions of fluctuations of fluence, flux density and total energy well follow the Tsallis q-Gaussian distribution. The q values keep steady around q ∼ 2 for different scale intervals, indicating a scale-invariant structure of the bursts. The statistical properties of FRB 121102 are very similar to that of the soft gamma repeater SGR J1550-5418. The underlying physical implications need to be further investigated.

scholarly journals A bimodal burst energy distribution of a repeating fast radio burst source

Nature ◽  
2021 ◽  
Vol 598 (7880) ◽  
pp. 267-271
Author(s):  
D. Li ◽  
P. Wang ◽  
W. W. Zhu ◽  
B. Zhang ◽  
X. X. Zhang ◽  
...  
Keyword(s):  
Energy Distribution ◽  
Radio Burst ◽  
Burst Source ◽  
Fast Radio Burst

scholarly journals Rotation Measure Evolution of the Repeating Fast Radio Burst Source FRB 121102

2021 ◽  
Vol 908 (1) ◽  
pp. L10 ◽  
Author(s):  
G. H. Hilmarsson ◽  
D. Michilli ◽  
L. G. Spitler ◽  
R. S. Wharton ◽  
P. Demorest ◽  
...  
Keyword(s):  
Radio Burst ◽  
Burst Source ◽  
Rotation Measure ◽  
Fast Radio Burst

scholarly journals Diverse polarization angle swings from a repeating fast radio burst source

Nature ◽  
2020 ◽  
Vol 586 (7831) ◽  
pp. 693-696 ◽  
Author(s):  
R. Luo ◽  
B. J. Wang ◽  
Y. P. Men ◽  
C. F. Zhang ◽  
J. C. Jiang ◽  
...  
Keyword(s):  
Radio Burst ◽  
Polarization Angle ◽  
Burst Source ◽  
Fast Radio Burst

scholarly journals Faint Repetitions from a Bright Fast Radio Burst Source

2019 ◽  
Vol 887 (2) ◽  
pp. L30 ◽  
Author(s):  
Pravir Kumar ◽  
R. M. Shannon ◽  
Stefan Osłowski ◽  
Hao Qiu ◽  
Shivani Bhandari ◽  
...  
Keyword(s):  
Radio Burst ◽  
Burst Source ◽  
Fast Radio Burst

scholarly journals Extremely band-limited repetition from a fast radio burst source

2020 ◽  
Vol 500 (2) ◽  
pp. 2525-2531 ◽  
Author(s):  
P Kumar ◽  
R M Shannon ◽  
C Flynn ◽  
S Osłowski ◽  
S Bhandari ◽  
...  
Keyword(s):  
Radio Burst ◽  
Broad Band ◽  
Ultra Wideband ◽  
Occurrence Rate ◽  
Burst Source ◽  
Broad Band Emission ◽  
Band Emission ◽  
Receiver System ◽  
Fast Radio Burst ◽  
Band Limited

ABSTRACT The fast radio burst (FRB) population is observationally divided into sources that have been observed to repeat and those that have not. There is tentative evidence that the bursts from repeating sources have different properties than the non-repeating ones. In order to determine the occurrence rate of repeating sources and characterize the nature of repeat emission, we have been conducting sensitive searches for repetitions from bursts detected with the Australian Square Kilometre Array Pathfinder (ASKAP) with the 64-m Parkes radio telescope, using the recently commissioned Ultra-wideband Low (UWL) receiver system, over a band spanning 0.7–4.0 GHz. We report the detection of a repeat burst from the source of FRB 20190711A. The detected burst is 1 ms wide and has a bandwidth of just 65 MHz. We find no evidence of any emission in the remaining part of the 3.3 GHz UWL band. While the emission bandwidths of the ASKAP and UWL bursts show ν−4 scaling consistent with a propagation effect, the spectral occupancy is inconsistent with diffractive scintillation. This detection rules out models predicting broad-band emission from the FRB 20190711A source and puts stringent constraints on the emission mechanism. The low spectral occupancy highlights the importance of sub-banded search methods in detecting FRBs.

scholarly journals Author Correction: A bimodal burst energy distribution of a repeating fast radio burst source

Nature ◽  
2021 ◽  
Author(s):  
D. Li ◽  
P. Wang ◽  
W. W. Zhu ◽  
B. Zhang ◽  
X. X. Zhang ◽  
...  
Keyword(s):  
Energy Distribution ◽  
Radio Burst ◽  
Burst Source ◽  
Fast Radio Burst

scholarly journals CHIME/FRB Detection of the Original Repeating Fast Radio Burst Source FRB 121102

2019 ◽  
Vol 882 (2) ◽  
pp. L18 ◽  
Author(s):  
A. Josephy ◽  
P. Chawla ◽  
E. Fonseca ◽  
C. Ng ◽  
C. Patel ◽  
...  
Keyword(s):  
Radio Burst ◽  
Burst Source ◽  
Fast Radio Burst
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