Scattering features and variability of the Crab pulsar
These are the Westerbork Synthesis Radio Telescope observation of the Crab pulsar analysed for the paper Scattering features and variability of the Crab pulsar published in the Monthly Notices for the Royal Astronomical Society. Each observation is fully averaged in time, and is averaged to eight frequency bands. The observations are at frequencies from 310 MHz to 380 MHz. The RFI has already been removed, and the dispersion measure (DM) has been corrected. The DM values for each observation can be found in the head, and also in the file file_information.csv. The data files are psrchive files, and the date of the observation is in the file name. If there is more than one observation on a given date, this is indicated by a -1 or -2 at the end of the date. The dates are also given in MJD in the file_information.csv file. ; The Westerbork Synthesis Radio Telescope is operated by the Netherlands Institute for Radio Astronomy (ASTRON) with support from The Netherlands Foundation for Scientific Research (NWO). LND and BWS acknowledge support from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (grant agreement No 694745).