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Table 1.
Data files processed to develop and demonstrate our algorithm.
Project | Observing | Sampling | File | Integration time | Known | Reference | Usage |
---|---|---|---|---|---|---|---|
semester | time (s) | count | per file (s) | signals | |||
P269 | Jan 2001 | 0.001 | 2251 | 8400 | Lorimer burst(FRB010724), and FRB010312 | Kaspi et al. (2016a) | Training and testing |
P269 | Oct 2000 | 0.001 | 951 | 2818 | – | Kaspi et al. (2016b) | Training |
P268 | Aug 1997 | 0.00025 | 4615 | 2100 | Single pulses fromknown pulsars | Lyne et al. (2012a) | Training and testing |
P268 | May 2001 | 0.00025 | 1820 | 2100 | FRB010621 | Lyne et al. (2012b) | Testing |
Notes. The testing data files are independent from the training data files.
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