Fast Radio Bursts (FRBs) are classified into repeaters and non-repeaters, with only a few percent of the observed FRB population from the Canadian Hydrogen Intensity Mapping Experiment (CHIME) confirmed as repeaters. However, this figure represents only a lower limit due to the observational biases, and the true fraction of repeaters remains unknown. Correcting for these biases uncovers a notable decline in apparently non-repeating FRB detection rate as the CHIME operational time increases. This finding suggests that a significant portion of apparently non-repeating FRBs could in fact exhibit repetition when observed over more extended periods. A simple population model infers that the true repeater fraction likely exceeds 50% with 99% conf...
FRB 20121102A is the first known fast radio burst (FRB) from which repeat bursts were detected, and ...
As more Fast Radio Bursts (FRBs) are being localised, we are learning that some fraction have persis...
Based on two very large samples of repeating fast radio bursts (FRBs), i.e. FRB 20121102A and FRB 20...
CHIME has now detected 18 repeating fast radio bursts (FRBs). We explore what can be learned about t...
According to the number of detected bursts, fast radio bursts (FRBs) can be classified into two cate...
CHIME has now detected 18 repeating fast radio bursts (FRBs). We explore what can be learned about t...
We have considered both non-CHIME and CHIME FRBs in the present study. Our robust conclusion is that...
Fast Radio Bursts (FRBs) are bursts of radio waves detected at great distances from space. Some FRBs...
A correlation between the intrinsic energy and the burst duration of non-repeating fast radio bursts...
About 900 fast radio burst (FRB) sources have been detected till now, among which 29 FRBs are found ...
Fast radio bursts are extragalactic, sub-millisecond radio impulses of unknown origin. Their dispers...
The fluence distribution of the fast radio burst (FRB) population (the 'source count' distribution, ...
Recently, CHIME/FRB project published its first fast radio burst (FRB) catalog (hereafter, Catalog 1...
Fast radio bursts (FRBs) are bright, millisecond-duration radio pulses of unknown origin. To date, o...
Several theories exist to explain the source of the bright, millisecond duration pulses known as fas...
FRB 20121102A is the first known fast radio burst (FRB) from which repeat bursts were detected, and ...
As more Fast Radio Bursts (FRBs) are being localised, we are learning that some fraction have persis...
Based on two very large samples of repeating fast radio bursts (FRBs), i.e. FRB 20121102A and FRB 20...
CHIME has now detected 18 repeating fast radio bursts (FRBs). We explore what can be learned about t...
According to the number of detected bursts, fast radio bursts (FRBs) can be classified into two cate...
CHIME has now detected 18 repeating fast radio bursts (FRBs). We explore what can be learned about t...
We have considered both non-CHIME and CHIME FRBs in the present study. Our robust conclusion is that...
Fast Radio Bursts (FRBs) are bursts of radio waves detected at great distances from space. Some FRBs...
A correlation between the intrinsic energy and the burst duration of non-repeating fast radio bursts...
About 900 fast radio burst (FRB) sources have been detected till now, among which 29 FRBs are found ...
Fast radio bursts are extragalactic, sub-millisecond radio impulses of unknown origin. Their dispers...
The fluence distribution of the fast radio burst (FRB) population (the 'source count' distribution, ...
Recently, CHIME/FRB project published its first fast radio burst (FRB) catalog (hereafter, Catalog 1...
Fast radio bursts (FRBs) are bright, millisecond-duration radio pulses of unknown origin. To date, o...
Several theories exist to explain the source of the bright, millisecond duration pulses known as fas...
FRB 20121102A is the first known fast radio burst (FRB) from which repeat bursts were detected, and ...
As more Fast Radio Bursts (FRBs) are being localised, we are learning that some fraction have persis...
Based on two very large samples of repeating fast radio bursts (FRBs), i.e. FRB 20121102A and FRB 20...