5th March 2018 
==============================================================

A) The maps from the original DES SV mass mapping papers using Kaiser-Squires: 
http://arxiv.org/abs/1504.03002
http://arxiv.org/abs/1505.01871

B) The maps from the paper:
“Improving Weak Lensing Mass Map Reconstructions using Gaussian and Sparsity Priors: Application to DES SV” 
https://arxiv.org/abs/1801.08945

==============================================================

A) 

des_sv_original_2015/${map_type}_${shear_pipeline}_${smoothing}_${pixel}.fits

map_type:
- k: kappa converted from ellipticity
- kg: weighted projected galaxy density map
* all maps are projected with a sinusoidal projection with 
reference RA at 71 deg
* for the kappa map, first extension is E-mode kappa, second is B-mode kappa, third is mask

shear_pipeline:
- im3shape v9 (flat v5)
- ngmix 011 (flat v5)
* photo-z from BPZ

smoothing:
RMS of Gaussian smoothing in arcmin

pixel:
size of pixel in arcmin

des_sv_original_2015/RA_des_sv_spte.fits
des_sv_original_2015/DEC_des_sv_spte.fits

RA/DEC coordinates for each pixel.

==============================================================

B) 

i) Kaiser-Squires with 10 arcminute Gaussian smoothing
des_sv_with_priors_2018/published_des_sv_map_ks_10am.fits

ii) Wiener filter reconstruction
des_sv_with_priors_2018/published_des_sv_map_wiener.fits

iii) GLIMPSE (sparse) reconstruction with λ=3.0
des_sv_with_priors_2018/published_des_sv_map_glimpse_l3.fits

all are HEALPIX format with NSIDE 1024 (as described in the paper)