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  Faraday rotation in Magellanic Bridge (Kaczmarek+, 2017)
Post annotation
1.J/MNRAS/467/1776/tableb1Table of the Faraday depth values for each polarized source used in our analysis (167 rows)

Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  Note (char) [*] Note (Note 1)   (meta.note)
  GLON deg Galactic longitude (pos.galactic.lon)
  GLAT deg Galactic latitude (
  P0 % Intrinsic polarization fraction (phys.polarization.linear)
  e_P0 % rms uncertainty on P0 (1σ) (stat.error)
  psi0 deg Intrinsic polarization angle (pos.posAng;phys.polarization)
  e_psi0 deg rms uncertainty on psi0 (1σ) (stat.error)
  phiraw rad/m2 Observed Faraday depth (phys.absorption.opticalDepth)
  e_phiraw rad/m2 rms uncertainty on phiraw (1σ) (stat.error)
  sigmaphi rad/m2 Faraday dispersion (instr.dispersion)
  e_sigmaphi rad/m2 rms uncertainty on sigmaphi (1σ) (stat.error)
  phicorr rad/m2 Faraday depth of each source once the Faraday rotation due to the MW foreground has been corrected for (phys.absorption.opticalDepth)
  e_phicorr rad/m2 rms uncertainty on phicorr (stat.error)
  _RA.icrs deg (n)(i) Right Ascension (ICRS, epoch 2000) computed by CDS (pos.eq.ra)
  _DE.icrs deg (n)(i) Declination (ICRS, epoch 2000) computed by CDS (pos.eq.dec)

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