Orateur
Caio Lima de Oliveira
(Universidade Estadual de Londrina)
Description
We present a per-galaxy weak lensing likelihood built directly on raw ellipticities and photometric P(z), modeling the unlensed ellipticity distribution while jointly fitting cluster mass and center via tangential and cross shear, with results from HSC and LSST Data Preview 1.
Auteur
Caio Lima de Oliveira
(Universidade Estadual de Londrina)