CHIME/Slow overview and pilot survey: A new backend to search for second-duration radio transients with the CHIME telescope
Sujay Mate, Kevin Luke, Yash Bhusare, Arvind Balasubramanian, Ziggy Pleunis, Paul Scholz, Shriharsh P. Tendulkar, Mohit Bhardwaj, Charanjot Brar, Fengqiu Adam Dong, Emmanuel Fonseca, B. M. Gaensler, Jason Hessels, Jeff Huang, Naman Jain, Ronniy C. Joseph, Victoria M. Kaspi

TL;DR
This paper introduces CHIME/Slow, a new backend for detecting second-duration radio transients with the CHIME telescope, presenting initial survey results, burst properties, and transient rate estimates.
Contribution
It presents the development and pilot testing of the CHIME/Slow pipeline for real-time second-duration radio transient detection, including initial survey results and transient rate estimation.
Findings
Detected nine radio bursts in 17 days of on-sky data.
Identified one new non-repeating and eight repeating bursts.
Estimated all-sky transient rate between 184 and 4556 bursts per day.
Abstract
We present an overview of CHIME/Slow, a real-time transient search backend under development to search for second-duration radio transients using the CHIME telescope, and results obtained from a pilot survey carried out using the prototype version of the search pipeline. The prototype CHIME/Slow pipeline was tested on archival data obtained in December 2022, January 2023 and February 2023 with a total on-sky time of 17 days with an instantaneous Field of View (FoV) of 13 deg . In this pilot survey, we detected nine bursts, one from a new non-repeating source and eight from the known hyperactive repeating source FRB 20220912A. Out of these nine bursts, two bursts from the repeater were not detected by CHIME/FRB, while the non-repeater was detected in the side-lobe of a beam in the CHIME/FRB exhibiting shorter pulse width and narrower bandwidth compared to the CHIME/Slow…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Astrophysics and Cosmic Phenomena · Pulsars and Gravitational Waves Research
