Yashar Hezaveh

Study reveals how distant galaxies influence each other and form stars.

This software simplifies and speeds up the analysis of astronomical images for researchers.

Innovative methods aim to improve measurements of the Universe's expansion rate.

PQMass measures the quality of generative models using probability mass estimation.

Researchers apply advanced methods to study RRLyrae stars and their light curves.

A new method enhances accuracy in astronomical data analysis through iterative learning.

Innovative approach connects N-body simulations to accurate galaxy counts efficiently.