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These tests can be done at the start of the pipeline, just by looking at input data.
They all focus on the PSF. There should be three star samples:
PSF stars
Reserved stars
All certain stars
Tests we need are:
Rowe statistics
PSF residual whisker plot (reserved stars) across FoV
Histogram of PSF size residuals
PSF size residual as function of magnitude
Intermediate Tests & Plots
These tests need some kind of calculated TXPipe intermediate or final quantities, often just the list of galaxies selected, sometimes tomographic bins, and sometimes other quantities. Many of them require the reponse factors to be correctly included.
Alpha/beta fit of shear to PSF
Mean shear plot across FoV
Gamma_t/x around chip centres
Gamma_t/x around field centres
Gamma_t/x around stars
Gamma_t/x around random points
Correlations between lensing map and systematics maps
Dependence of source density and ellipticity on observing conditions
Dependence of source density and ellipticity on n_visit
Star-Galaxy correlation function
B-modes
B-mode mass aperture statistic
gamma_x around lenses
Difference in corr functions when split by S/N
Difference in corr functions when split by systematic quantities
Difference in corr functions when split by chip location
Difference in corr functions when split by chip number
The text was updated successfully, but these errors were encountered:
It's ocurred to me that the best way to do correlation functions with size and SNR splits is to just re-run the entire pipeline with different cuts, since that will do everything including computing the new n(z) values. So I'll call that complete.
Early Tests & Plots
These tests can be done at the start of the pipeline, just by looking at input data.
They all focus on the PSF. There should be three star samples:
Tests we need are:
Intermediate Tests & Plots
These tests need some kind of calculated TXPipe intermediate or final quantities, often just the list of galaxies selected, sometimes tomographic bins, and sometimes other quantities. Many of them require the reponse factors to be correctly included.
The text was updated successfully, but these errors were encountered: