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- W2896427903 abstract "LOFAR achieves high time resolution (< 1 s samples) using its various beam-formed modes. These modes are vital for observations of pulsars, fast radio transients, the Sun, (exo)planets, flare stars and dynamic spectra of scintillating sources—to name a few examples. Here we describe the observing modes and tools available to process raw LOFAR beam-formed data, including the standard pulsar pipeline (‘PulP’; pulppy) and further analysis—with a focus on pulsar dedispersion, folding, RFI excision, polarimetry and searching. We also describe a general purpose dynamic spectrum toolkit." @default.
- W2896427903 created "2018-10-26" @default.
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- W2896427903 date "2018-01-01" @default.
- W2896427903 modified "2023-09-23" @default.
- W2896427903 title "High Time Resolution with LOFAR" @default.
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- W2896427903 doi "https://doi.org/10.1007/978-3-319-23434-2_14" @default.
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