Power Spectrum with MAXI GSC data

Data processed until 16 07 2017 14:35:09 (JST)

All sources (400)

  • The PSDs are calculated by discrete fourier transformation.
  • The data gaps are linearly interpolated.
  • The PSDs are normalized by dividing by the square of the average intensity (= NPSD).
  • The light curve datas are downloaded from http://maxi.riken.jp/top/.
  • The light curve data from 55058MJD are processed.
  • The peak at 1.65e-7 Hz (=70 days) is artificial due to presession of the ISS’s rotational axis. The scan direction and location on cameras change with this period.