The Dark Energy Spectroscopic Instrument (DESI) completed its 5 month Survey Validation
in 2021 May. Spectra of stellar and extragalactic targets from Survey Validation constitute …

We propose an effective model to describe the bias induced on cosmological observables
by Laniakea, the gravitational supercluster hosting the Milky Way, which was defined using …

The detailed nature of dark energy remains a mystery, leaving the possibility that its effects
might be explained by changes to the laws of gravity on large scales. The peculiar velocities …

We infer the growth of large scale structure over the redshift range $0.4\lesssim z\lesssim 1$
from the cross-correlation of spectroscopically calibrated Luminous Red Galaxies (LRGs) …

We use deep spectroscopy from the SAMI (Sydney-AAO Multi-object Integral) Galaxy Survey
to explore the precision of the fundamental plane (FP) of early-type galaxies as a distance …

Measurements of the peculiar velocities of large samples of galaxies enable new tests of the
standard cosmological model, including determination of the growth rate of cosmic structure …

We present the 2020 version of the Siena Galaxy Atlas (SGA-2020), a multiwavelength
optical and infrared imaging atlas of 383,620 nearby galaxies. The SGA-2020 uses optical …

We explore the science prospects of a 14,000 deg $^ 2$ Kinematic Lensing (KL) survey with
the Dark Energy Spectroscopic Instrument (DESI) and overlapping imaging surveys. KL …

Peculiar velocities are an important probe of the mass distribution in the Universe and the
growth rate of structure, directly measuring the effects of gravity on the largest scales and …

Peculiar motion of galaxies probes the structure growth in the universe. In this study, we
employ the galaxy stellar mass-binding energy (massE) relation with only two nuisance …