The distortions are tiny, but starting in 2000, astronomers managed to detect the effect, which is known as
cosmological weak lensing, in surveys of thousands of galaxies.
Not exact matches
Dark Energy Survey year 1 results:
Cosmological constraints from galaxy clustering and
weak lensing.
In addition to Gruen, who led the
weak lensing working group, and Wechsler, whose group provided realistic simulations of the survey critical to testing several aspects of the
cosmological analysis, a large number of KIPAC scientists, postdoctoral fellows, graduate students and alumni have made crucial contributions to DES — from building the instrument to developing theory and simulations and analyzing the data.
Astronomers have found a number of uses for ESI, from observing the
cosmological effects of
weak gravitational
lensing to searching for the most metal - poor stars in our galaxy.