A census of the pulsar population observed with the international LOFAR station FR606 at low frequencies (25–80 MHz)

dc.contributor.authorSerylak, M.
dc.contributor.authorBondonneau, L.
dc.contributor.authorGrießmeier, J.-M.
dc.date.accessioned2021-02-15T12:26:47Z
dc.date.available2021-02-15T12:26:47Z
dc.date.issued2020
dc.description.abstractontext. To date, only 69 pulsars have been identified with a detected pulsed radio emission below 100 MHz. A LOFAR-core LBA census and a dedicated campaign with the Nançay LOFAR station in stand-alone mode were carried out in the years 2014–2017 in order to extend the known population in this frequency range. Aims. In this paper, we aim to extend the sample of known radio pulsars at low frequencies and to produce a catalogue in the frequency range of 25–80 MHz. This will allow future studies to probe the local Galactic pulsar population, in addition to helping explain their emission mechanism, better characterising the low-frequency turnover in their spectra, and obtaining new information about the interstellar medium through the study of dispersion, scattering, and scintillation. Methods. We observed 102 pulsars that are known to emit radio pulses below 200 MHz and with declination above −30°. We used the Low Band Antennas (LBA) of the LOw Frequency ARray (LOFAR) international station FR606 at the Nançay Radio Observatory in stand-alone mode, recording data between 25 and 80 MHz.en_US
dc.identifier.citationSerylak, M. et al. (2020). A census of the pulsar population observed with the international LOFAR station FR606 at low frequencies (25–80 MHz). Astronomy & Astrophysics, 635, A76en_US
dc.identifier.issn1432-0746
dc.identifier.urihttps://doi.org/10.1051/0004-6361/201936829
dc.identifier.urihttp://hdl.handle.net/10566/5932
dc.language.isoenen_US
dc.publisherEDP Sciencesen_US
dc.subjectPulsars: generalen_US
dc.subjectTelescopesen_US
dc.subjectISM: generalen_US
dc.subjectLOFAR stationen_US
dc.titleA census of the pulsar population observed with the international LOFAR station FR606 at low frequencies (25–80 MHz)en_US
dc.typeArticleen_US

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