Added error on star polarization and contrast curves for PDI

• Added computation of statistical uncertainty (photon and background noise) on measured star polarization in PDI part
• Added contrast curves for the detection of polarized extended sources and polarized point source with PDI

Added ADI+PCA for total intensity images in pupil-tracking mode

• Added angular differential imaging (ADI) including principal component analysis (PCA) of total intensity images for pupil-tracking observations
• Added mean combination of ADI final images to command-line option

Expressing images in contrast/arcsec^2 or Jansky/arcsec^2, restructured code and configuration file

• Added analysis of master flux frames to enable the user to express the final images in contrast/arcsec^2 or Jansky/arcsec^2
• Restructered code and configuration file to allow for the separate execution of pre-processing, polarimetric differential imaging (previously referred to as post-processing) and angular differential imaging
• Added plot of center coordinates of center frames vs time
• Added possibility to open documentation through terminal command "irdap --website"
• Confirmed that polarimetric data with dithering applied is correctly reduced

Added command-line option to mean-combine final images of different observation blocks

Added command-line option to mean-combine final images of different observation blocks

Added possibility to reduce data with narrowband filters

Added the possibility to reduce data taken with the narrowband filters using the existing model of the broadband filters

Ks P0-90 static flat + changes to annulus definition

• Changed the definition of the tuple of the input parameters annulus_star, annulus_background and flux_annulus_background: width is replaced by outer_radius and the definition of start_angle and end_angle is now the same as in DS9
• Replaced static flat in Ks by one with P0-90 inserted

First release of IRDAP

First official release of IRDAP + documentation on PyPI and GitHub