| Autor: |
Sheikh, Sofia Z, Farah, Wael, Pollak, Alexander W, Siemion, Andrew P V, Chamma, Mohammed A, Cruz, Luigi F, Davis, Roy H, DeBoer, David R, Gajjar, Vishal, Karn, Phil, Kittling, Jamar, Lu, Wenbin, Masters, Mark, Premnath, Pranav, Schoultz, Sarah, Shumaker, Carol, Singh, Gurmehar, Snodgrass, Michael |
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| Zdroj: |
Monthly Notices of the Royal Astronomical Society; Feb2024, Vol. 527 Issue 4, p10425-10439, 15p |
| Abstrakt: |
FRB 20220912A is a repeating Fast Radio Burst (FRB) that was discovered in Fall 2022 and remained highly active for several months. We report the detection of 35 FRBs from 541 h of follow-up observations of this source using the recently refurbished Allen Telescope Array, covering 1344 MHz of bandwidth primarily centred at 1572 MHz. All 35 FRBs were detected in the lower half of the band with non-detections in the upper half and covered fluences from 4–431 Jy-ms (median = 48.27 Jy-ms). We find consistency with previous repeater studies for a range of spectrotemporal features including: bursts with downward frequency drifting over time; a positive correlation between bandwidth and centre frequency; and a decrease in sub-burst duration over time. We report an apparent decrease in the centre frequency of observed bursts over the two months of the observing campaign (corresponding to a drop of 6.21 ± 0.76 MHz per d). We predict a cut-off fluence for FRB 20220912A of F max ≲ 104 Jy-ms, for this source to be consistent with the all-sky rate, and find that FRB 20220912A significantly contributed to the all-sky FRB rate at a level of a few per cent for fluences of ∼100 Jy-ms. Finally, we investigate characteristic time-scales and sub-burst periodicities and find (a) a median inter-subburst time-scale of 5.82 ± 1.16 ms in the multi-component bursts and (b) no evidence of strict periodicity even in the most evenly spaced multi-component burst in the sample. Our results demonstrate the importance of wideband observations of FRBs, and provide an important set of observational parameters against which to compare FRB progenitor and emission mechanism models. [ABSTRACT FROM AUTHOR] |
| Databáze: |
Complementary Index |
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