2012/05/14 by Peeyush Prasad, Prasad, Peeyush, Stefan J. Wijnholds +1 · 1 citation
Engineering · Physics and Astronomy · #Adaptive optics and wavefront sensing #Antenna Design and Optimization #FOS: Physical sciences #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Radio Astronomy Observations and Technology
paper · pdf · doi:10.48550/arxiv.1205.3056
openalex publication_date 2012/05/14 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The AARTFAAC project aims to implement an All-Sky Monitor (ASM), using the Low Frequency Array (LOFAR) telescope. It will enable real-time, 24x7 monitoring for low frequency radio transients over most of the sky locally visible to the LOFAR at timescales ranging from milliseconds to several days, and rapid triggering of follow-up observations with the full LOFAR on detection of potential transient candidates. These requirements pose several implementation challenges: imaging of an all-sky field of view, low latencies of processing, continuous availability and autonomous operation of the ASM. The first of these has already resulted in the correlator for the ASM being the largest in the world in terms of its number of input channels. It will generate ∼ 1.5 ⋅ 105 correlations per second per spectral channel when built. Test observations using existing LOFAR infrastructure were carried out to quantify and constrain crucial instrumental design criteria for the ASM. In this paper, we present an overview of the AARTFAAC data processing pipeline and illustrate some of the aforementioned challenges by showing all-sky images obtained from one of the test observations. These results provide quantitative estimates of the capabilities of the instrument.