, used since 2006 to report transient astronomical events. This system alerts observatories worldwide when FRBs occur, giving them the chance to train their instruments on the source and conduct follow-up observations.
Nevertheless, CHIME has still had one limitation: its inability to identify an FRB’s origin with any precision. CHIME is hardly alone in this, as the transient nature of FRBs makes them extremely difficult to study and is the reason why only a few have been traced back to their point of origin. The addition of new outriggers to radio observatories partnered with the DRAO will enable this for the first time.
Patrick Boyle, the Senior Project Manager for the CHIME/FRB Outriggers project and Senior Academic Associate in the Department of Physics at McGill University, explained in a recent SETI Institute“The CHIME telescope can currently locate the position of a fast radio burst to a patch of sky equivalent to the size of the full Moon. With the addition of the three new outrigger telescopes, this patch of sky can be reduced to the size of a quarter held at roughly 40 km.
– and the Green Bank Observatory is also expected to enhance CHIME’s abilities to study FRBs. On May 18th, 2021, researchers at ATA made the first-ever detection of an FRB with their radio telescopes. This was the bright double-peaked repeating FRB known asIn recent years, the ATA has been undergoing a refurbishment program to upgrade its telescope feeds and digital signal processing system to improve its sensitivity and capabilities.
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