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J/MNRAS/520/314
  Polarization geometry of observed LOFAR pulsars (Wahl+, 2023)
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1.J/MNRAS/520/314/tablea2The physical spin down parameters of our pulsars sample (133 rows)

 
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ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  Name (char) Pulsar name designation as JHHMM+DDMM (Pulsar) (meta.id;meta.main)
  P s Barycentric period of the pulsar (P) (time.period)
  dP/dt 10-15 (n) Period derivative spin-down rate (dP/dt) (arith.rate;time.period)
  dE/dt 10+25W (n) The spin-down energy loss rate (dE/dt) (phys.energy)
  tau Myr (n) Pulsar scattering spin-down age as P/[dP/dt] ({tau}) (time.age)
  Bsurf 10+12gauss(n) The surface magnetic flux density of the pulsar (Bsurf) (phys.magField)
  B12/P2  (n) The pulsar acceleration potential parameter as (|Bsurf|*10–12/P2) as the ability of the pulsar to accelerate charged particles (B12/P2) (phys.acceleration)
  1/Q  (n) The reciprocal Q parameter as 1/Q = 0.5(dP/dt)0.4–15/P–1.1 of Beskin et al. 1993ppm..book.....B (1/Q) (stat.param)

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