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      LOFAR PSR low-frequency Faraday rotation measures

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      Creators
      Sobey, C
      Bilous, A.V.
      Grießmeier, J.M.
      Hessels, J.W.T.
      Karastergiou, A.
      Keane, E.F.
      Kondratiev, V.I.
      Kramer, M.
      Michilli, D.
      Noutsos, A.
      Pilia, M.
      Polzin, E.J.
      Stappers, B.W.
      Tan, C.M.
      Leeuwen, J. van
      Verbiest, J.P.W.
      Weltevrede, P.
      Heald, G.
      Alves, M.I.R.
      Carretti, E.
      Enßlin, T.
      Haverkorn, M.
      Iacobelli, M.
      Reich, W.
      Eck, C.L. van
      Date of Archiving
      2019
      Archive
      VizieR Online
      Related links
      http://vizier.cfa.harvard.edu/viz-bin/VizieR?-source=J/MNRAS/484/3646
      Related publications
      Low-frequency Faraday rotation measures towards pulsars using LOFAR: probing the 3D Galactic halo magnetic field  
      Publication type
      Dataset
      Access level
      Open access
      Please use this identifier to cite or link to this item: https://hdl.handle.net/2066/201824   https://hdl.handle.net/2066/201824
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      Organization
      Astrophysics
      Audience(s)
      Astronomy, astrophysics
      Key words
      Pulsars; Magnetic fields
      Abstract
      The data in table RMcatcsv.dat presents the results (ionosphere-corrected) RMs determined towards 136 pulsars, using 110-190MHz LOFAR observations taken between 2012 December to 2014 November. We determined the RMs towards 117 pulsars in the non-recycled pulsar census (Bilous et al., 2016A&A...591A.134B) and 19 pulsars in the MSP census (Kondratiev et al., 2016A&A...585A.128K).
      This item appears in the following Collection(s)
      • Datasets [1229]
      • Faculty of Science [31868]
       
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