The CRAFT coherent (CRACO) upgrade I: System description and results of the 110-ms radio transient pilot survey
Ziteng Wang, K. W. Bannister, Vivek Gupta, Xiao-Dong Deng, M. A. Pilawa, J. Tuthill, J. D. Bunton, Chris Flynn, Marcin Glowacki, A. Jaini, YongKeun Lee, E. Lenc, J. Lucero, Aeri M. Paek, Raghu Radhakrishnan, Nithyanandan Thyagarajan, P. A. Uttarkar, Y. Wang, N. D. R. Bhat, C. James, Vanessa A. Moss, Tara Murphy, J. E. Reynolds, R. M. Shannon, L. G. Spitler, A. K. Tzioumis, Manisha Caleb, Adam T. Deller, Alexa C. Gordon, Lachlan Marnoch, S. D. Ryder, Sunil Simha, C. S. Anderson, Lewis Ball, David Brodrick, F. R. Cooray, N. Gupta, Douglas B. Hayman, A. Ng, Sarah E. Pearce, Chris Phillips, M. A. Voronkov, T. Westmeier
Abstract
Abstract We present the first results from a new backend on the Australian Square Kilometre Array Pathfinder, the Commensal Realtime ASKAP Fast Transient COherent (CRACO) upgrade. CRACO records millisecond time resolution visibility data, and searches for dispersed fast transient signals including fast radio bursts (FRB), pulsars, and ultra-long period objects (ULPO). With the visibility data, CRACO can localise the transient events to arcsecond-level precision after the detection. Here, we describe the CRACO system and report the result from a sky survey carried out by CRACO at 110-ms resolution during its commissioning phase. During the survey, CRACO detected two FRBs (including one discovered solely with CRACO, FRB 20231027A), reported more precise localisations for four pulsars, discovered two new RRATs, and detected one known ULPO, GPM J1839 $-$ 10, through its sub-pulse structure. We present a sensitivity calibration of CRACO, finding that it achieves the expected sensitivity of 11.6 Jy ms to bursts of 110 ms duration or less. CRACO is currently running at a 13.8 ms time resolution and aims at a 1.7 ms time resolution before the end of 2024. The planned CRACO has an expected sensitivity of 1.5 Jy ms to bursts of 1.7 ms duration or less and can detect $10\times$ more FRBs than the current CRAFT incoherent sum system (i.e. 0.5 $-$ 2 localised FRBs per day), enabling us to better constrain the models for FRBs and use them as cosmological probes.