VIA lecture by Daniel Gruen "Cosmology from Weak Lensing in the Dark Energy Survey" waas given on 01.12.2017.
It's presentation is attached.
The following questions and comments were put in discussion
Houri Ziaeepour: The error on the redshift as you showed is ~1.5%. I don't understand how you can give an error of order 0.001 for w .
Houri Ziaeepour: But your value of H0 is quite far from SN.
Houri Ziaeepour: Probably a better understanding of differences between CMB and DES results would help. For all parameters.