Corrected error due to numpy.int deprecated and warning on IP model

Corrected error due to numpy.int deprecated and warning on IP model

Corrected an error due to a scikit-image function being deprecated

Corrected an error due to a scikit-image function being deprecated
Changed to new ESO e-mail address

Updated code so that it correctly handles the change of the header names INS4 DROT2 BEGIN and INS4 DROT3 BEGIN to INS4 DROT2 START and INS4 DROT3 START in the FITS files

Updated code so that it correctly handles the change of the header names INS4 DROT2 BEGIN and INS4 DROT3 BEGIN to INS4 DROT2 START and INS4 DROT3 START in the FITS files

Corrected a bug that prevented reductions to be performed when dark and flat files are included in the raw subdirectory

Corrected a bug that prevented reductions to be performed when dark and flat files are included in the raw subdirectory

Added command-line option (irdap --print) to toggle printing of log statements in the terminal

Added command-line option (irdap --print) to toggle printing of log statements in the terminal

Implemented two new configuration parameters for the computation of the final Q-, U-, I_Q- and I_U-images

• Implemented two new configuration parameters (combination_method_polarization and combination_method_intensity) for the computation of the final Q-, U-, I_Q- and I_U-images. The Q- and U-images can now be computed using least squares (as was previously the only option), the median and the trimmed mean. The I_Q- and I_U-images can be computed from the mean (as was previously the only option), the median and the trimmed mean
• Old configuration files that do not have these parameters can still be used: IRDAP automatically uses the default least squares and mean options if these new configuration parameters are missing from the configuration file
• Some minor additional improvements

Clarified in log file which uncertainty to quote in papers + updates check + correct ADS links

• Put temporal uncertainty as uncertainty of the star polarization in the log file, added the accuracy of the Mueller matrix model and clarified which uncertainty to quote in papers.
• Made IRDAP check for updates when run
• Implemented correct link to ADS of van Holstein et al. (2020) in program and documentation

Corrected computation of HWP angle and bug in computation of polarimetric efficiency + various minor improvements to log file and documentation

• Clarified meaning of standard deviation of fitted center coordinates in log file
• Very minor correction to computation of HWP angle from headers
• Corrected minor bug when computing polarimetric efficiency when the number of Q and U cycles is unequal
• Added warning when spread of star polarization per HWP cycle is large and suggest to try normalized double difference

Added polarimetric efficiency to plot and log + corrections of 2 minor bugs

• Added polarimetric efficiency to crosstalk/transmission plot, a print statement with the range of the polarimetric efficiency of the observations, and a warning in case of low polarimetric efficiency
• Corrected a bug in the checks of flux_annulus_star
• Corrected a bug that when mean combining ADI+PCA-images only the first frame of the cube was written to the FITS-files

Correction of minor bug

• Corrected bug introduced in v1.2.0 with computation of DoLP and AoLP of star when there is an unequal number of Q and U measurements