Observing pulsars and fast transients with LOFAR
B. W. Stappers, J. W. T. Hessels, A. Alexov, K. Anderson, T. Coenen,, T. Hassall, A. Karastergiou, V. I. Kondratiev, M. Kramer, J. van Leeuwen, J., D. Mol, A. Noutsos, J. W . Romein, P. Weltevrede, R. Fender, R. A. M. J., Wijers, L. B\"ahren, M. E. Bell, J. Broderick, E. J. Daw

TL;DR
LOFAR is a cutting-edge low-frequency radio telescope that enhances pulsar and transient observations, offering new insights into pulsar science and fast radio transient phenomena at frequencies 10-240MHz.
Contribution
This paper introduces LOFAR's design and capabilities for low-frequency pulsar and transient observations, highlighting its potential to revolutionize radio astronomy at these frequencies.
Findings
Demonstrated LOFAR's high-time-resolution observation capabilities
Presented initial results from commissioning observations
Outlined data reduction pipelines for pulsar and transient detection
Abstract
Low frequency radio waves, while challenging to observe, are a rich source of information about pulsars. The LOw Frequency ARray (LOFAR) is a new radio interferometer operating in the lowest 4 octaves of the ionospheric "radio window": 10-240MHz, that will greatly facilitate observing pulsars at low radio frequencies. Through the huge collecting area, long baselines, and flexible digital hardware, it is expected that LOFAR will revolutionize radio astronomy at the lowest frequencies visible from Earth. LOFAR is a next-generation radio telescope and a pathfinder to the Square Kilometre Array (SKA), in that it incorporates advanced multi-beaming techniques between thousands of individual elements. We discuss the motivation for low-frequency pulsar observations in general and the potential of LOFAR in addressing these science goals. We present LOFAR as it is designed to perform…
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