Pulsar scintillation studies with LOFAR I. The census

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dc.contributor.authorWu, Ziwei
dc.contributor.authorVerbiest, Joris P. W.
dc.contributor.authorSerylak, Maciej
dc.date.accessioned2022-08-19T10:22:53Z
dc.date.available2022-08-19T10:22:53Z
dc.date.issued2022
dc.description.abstractInterstellar scintillation (ISS) of pulsar emission can be used both as a probe of the ionized interstellar medium (IISM) and cause corruptions in pulsar timing experiments. Of particular interest are so-called scintillation arcs which can be used to measure time-variable interstellar scattering delays directly, potentially allowing high-precision improvements to timing precision.The primary aim of this study is to carry out the first sizeable and self-consistent census of diffractive pulsar scintillation and scintillation-arc detectability at low frequencies, as a primer for larger-scale IISM studies and pulsar-timing related propagation studies with the LOw-Frequency ARray (LOFAR) High Band Antennae (HBA).en_US
dc.identifier.citationWu, Z. et al. (2022). Pulsar scintillation studies with LOFAR I. The census. Astronomy and Astrophysics, 663, A116. https://doi.org/10.1051/0004-6361/202142980en_US
dc.identifier.issn2329-1265
dc.identifier.urihttps://doi.org/10.1051/0004-6361/202142980
dc.identifier.urihttp://hdl.handle.net/10566/7753
dc.language.isoenen_US
dc.publisherHans Publishersen_US
dc.subjectAstrophysicsen_US
dc.subjectAstronomyen_US
dc.subjectPulsarsen_US
dc.subjectAntenna networken_US
dc.subjectRadio interferometeren_US
dc.titlePulsar scintillation studies with LOFAR I. The censusen_US
dc.typeArticleen_US

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