HSC year 1 real space cosmic shear (reprocess)

Please cite the paper if you are using the reprocessed HSC cosmic shear data: https://ui.adsabs.harvard.edu/abs/2022arXiv221203257Z/abstract

Note the constrain has $0.15 \sigma$ difference in $\Omega_m$ compared to the official HSC year 1 analysis shown in this paper: https://arxiv.org/pdf/1906.06041.pdf

likelihood

Run the analysis pipeline under this directory:

cosmosis config.ini

redshift distribution $n(z)$

The redshift distribution can be found in this notebook

PSF systematics

The PSF shape-shape residual correlation functions can be found in this notebook

chain

You can plot the output chain following this notebook