A highly magnetized environment in a pulsar binary system

A highly magnetized environment in a pulsar binary system <strong>Data availability:</strong> IPV and DM, RM variations used for Fig 1 (Demo how to read the code and plot: plot_Fig1.py) DM_Icut_60s_140114.txt, DM_Icut_60s_200621.txt, RM_140114_20s_rmfit.txt,RM_200621_20s_rmfit.txt, ILV_140114_20s.npy, ILV_200621_20s.npy A full table of DM and RM variations (duplicated with the txt files, but with better readability): Li_DM_RM_Ter5A.xlsx Calibrated full stokes data with frequency information for Fig 2 (in psrfit format, can be read in with standard psrchive commands): VEGAS_Ter5A_200621_0001.zap.E2.calib.rot.f32 <strong>Code availability</strong> <em>The basic process of the raw data and DM, RM fitting:</em> DSPSR (http://dspsr.sourceforge.net) PSRCHIVE (http://psrchive.sourceforge.net) <em>Modeling and fitting:</em> https://github.com/dongzili/Pol_prop_fitting NOTICE: If there are updated data due to new demands, the information or new URL will be posted in https://github.com/dongzili/Pol_prop_fitting