PuMaII: A wide band pulsar machine for the WSRT

TL;DR

PuMa II is a flexible, wide bandwidth pulsar processing system at WSRT that enables high-resolution, real-time data analysis for advanced pulsar research.

Contribution

It introduces a new pulsar backend system with significantly increased bandwidth and coherent dedispersion capabilities at WSRT.

Findings

Doubled the bandwidth for pulsar observations.

Enabled coherent dedispersion over 160 MHz bandwidth.

Achieved a maximum time resolution of 50ns.

Abstract

The Pulsar Machine II (PuMa II) is the new flexible pulsar processing backend system at the Westerbork Synthesis Radio Telescope (WSRT), specifically designed to take advantage of the upgraded WSRT. The instrument is based on a computer cluster running the Linux operating system, with minimal custom hardware. A maximum of 160 MHz analogue bandwidth sampled as 8X20 MHz subbands with 8-bit resolution can be recorded on disks attached to separate computer nodes. Processing of the data is done in the additional 32-nodes allowing near real time coherent dedispersion for most pulsars observed at the WSRT. This has doubled the bandwidth for pulsar observations in general, and has enabled the use of coherent dedispersion over a bandwidth eight times larger than was previously possible at the WSRT. PuMa II is one of the widest bandwidth coherent dedispersion machines currently in use and has a maximum time resolution of 50ns. The system is now routinely used for high precision pulsar timing studies, polarization studies, single pulse work and a variety of other observational work.