The Southern-sky MWA Rapid Two-metre (SMART) pulsar survey -- I. Survey design and processing pipeline

• Published in: arXiv.org 2023-02
• Main Authors: Bhat, N D R, Swainston, N A, McSweeney, S J, Xue, M, Meyers, B W, Kudale, S, Dai, S, Tremblay, S E, W van Straten, Shannon, R M, Smith, K R, Sokolowski, M, Ord, S M, Sleap, G, Williams, A, Hancock, P J, Lange, R, Tocknell, J, Johnston-Hollitt, M, Kaplan, D L, Tingay, S J, Walker, M
• Format: Article
• Language: English
• Subjects: Arrays; Beamforming; Data collection; Declination; Dwell time; Electric potential; Millisecond pulsars; Pipeline design; Pulsars; Reprocessing; Searching; Sky surveys (astronomy); Southern sky; Voltage
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.2302.11911

We present an overview of the Southern-sky MWA Rapid Two-metre (SMART) pulsar survey that exploits the MWA's large field of view and voltage capture system to survey the sky south of 30 degree in declination for pulsars and fast transients in the 140-170 MHz band. The survey is enabled by the advent of the Phase II MWA's compact configuration, which offers an enormous efficiency in beam-forming and processing costs, thereby making an all-sky survey of this magnitude tractable with the MWA. Even with the long dwell times of the survey (4800 s), data collection can be completed in < 100 hours of telescope time, while still retaining the ability to reach a limiting sensitivity of ~2-3 mJy. Each observation is processed to generate ~5000-8000 tied-array beams that tessellate the full ~610 square degree field of view, which are then processed to search for pulsars. The voltage-capture recording allows a multitude of post hoc processing options including the reprocessing of data for higher time resolution. Due to the substantial computational cost in pulsar searches at low frequencies, processing is undertaken in multiple passes: in the first pass, a shallow survey is performed, where 10 minutes of each observation is processed, reaching about one-third of the full search sensitivity. Here we present the system overview and initial results. Further details including first pulsar discoveries and a census of low-frequency detections are presented in a companion paper. Future plans include deeper searches to reach the full sensitivity and acceleration searches to target binary and millisecond pulsars. Simulation analysis forecasts ~300 new pulsars upon the completion of full processing. The SMART survey will also generate a complete digital record of the low-frequency sky, which will serve as a valuable reference for future pulsar searches planned with the low-frequency Square Kilometre Array.