Change history

  • New version 1.2 (25/05/20): new tables for systematic errors, random noise can vary with mask shapes and mask updates, amplitude of the drift can be controlled by the parameter Systematic/DriftLevel, mask updates are flagged. For more details see the release notes.
  • 1.1 (03/02/20): Some Python3 compatibility issues corrected. New option “-m” to generate merged light-curves, new option “-M” to perform Monte-Carlo simulations
  • 1.0 (05/09/19): Implementation of the V-P color-magnitude relation from Marchiori et al (2019). The option -f saves now each individual light-curves. Oscillations can be turned off. New format for the input file (YAML). PLATO NSR values are now available down to magnitude P=15.6.
  • 0.9 (20/05/19): the NSR table was incorrectly interpolated. V mangitudes ranging between 12 and 13 were affected.
  • 0.85 (23/03/19): minor changes to be make the code fully compatible with python3
  • 0.8 (23/02/19): systematic errors are now modelled and simulated in the time domain. The jumps induced by the quasi-regular mask updates are now included. Version corresponding to the published paper Samadi et al (2019, A&A, 624, 117)
  • 0.7 (10/12/18): inclusion of PLATO systematic errors and random noise as a function of the star V magnitude
  • 0.6: minor problems fixed (missing file, link problem)
  • 0.5: can perform simulation for a given input set of theoretical frequencies (i.e. from a given .gsm file) ; new parameters included in the configuration file .yaml ; various minor improvements
  • 0.4: minor changes
  • 0.3: first working version

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