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MAD in a BHXRB MAXI J1820+070

Abstract

All the necessary data and scripts to reproduce You B., et al., (2023)

Description

  • Multi-wavelengths observation data folder contains the data points which are plotted in Fig. 1、2、4, and Fig. S7、S8.

  • Time-delay folder contains

    (i) the script piccf_mc.c which uses the data points in Fig. 2 to determine the lags between flares of different wavelengths;

    (ii) the script iccf.py is used to plot the relevant results in Fig. S1.

  • Formation of a MAD folder contains one script code.ipynb which is used to plot Fig. S3-S6. The source code which simulates the magnetic field is also provided.

  • Simulation of a DIM folder contains the source code which simulates the DIM.

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  • Jupyter Notebook 48.2%
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  • C 11.3%
  • Python 5.5%