A highly magnetized environment in a pulsar binary system

A highly magnetized environment in a pulsar binary system

Data availability:

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

Code availability

The basic process of the raw data and DM, RM fitting:

DSPSR (http://dspsr.sourceforge.net) PSRCHIVE (http://psrchive.sourceforge.net)

Modeling and fitting:

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

脉冲星双星系统中的强磁化环境

数据可用性：
用于绘制图1的IPV、DM（色散量，Dispersion Measure）、RM（旋转测度，Rotation Measure）变化数据（代码读取与绘图演示脚本：plot_Fig1.py），包含以下文件：
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

包含DM与RM变化量的完整数据表（与上述txt文件内容一致，但可读性更佳）：Li_DM_RM_Ter5A.xlsx

用于绘制图2的带频率信息的校准全Stokes（斯托克斯）数据（格式为psrfit，可通过标准psrchive命令读取）：VEGAS_Ter5A_200621_0001.zap.E2.calib.rot.f32

代码可用性：
原始数据处理与DM、RM拟合的基本流程依托以下工具完成：
DSPSR（http://dspsr.sourceforge.net）与PSRCHIVE（http://psrchive.sourceforge.net）

建模与拟合：
https://github.com/dongzili/Pol_prop_fitting

注意：若因新需求更新数据，相关说明或新链接将发布于https://github.com/dongzili/Pol_prop_fitting