activity
20032022
most citedAction Dynamics of the Local Supercluster

122 citations · 536 across the 11 of their papers we have counts for

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Showing astro-ph.COShow all

11 papers · 1 filter

astro-ph.CO20229 cited

Galaxy flows within 8,000 km/s from Numerical Action methods

Edward Shaya, R. Brent Tully, Daniel Pomarède +1

The trajectories since z=4 of systems of galaxies (`halos') with cz < 8,000 km/s are found through Numerical Action reconstructions. A set of 9,719 halos from a 2MASS group catalog…

astro-ph.CO202028 cited

Cosmicflows-3: The South Pole Wall

Daniel Pomarede, R. Brent Tully, Romain Graziani +3

Velocity and density field reconstructions of the volume of the universe within 0.05c derived from the Cosmicflows-3 catalog of galaxy distances has revealed the presence of a fila…

astro-ph.CO2019101 cited

Cosmicflows-3: Two DistanceVelocity Calculators

Ehsan Kourkchi, Helene M. Courtois, Romain Graziani +4

Tools are provided at the Extragalactic Distance Database website that provide relationships between the distances and velocities of galaxies based on smoothed versions of the velo…

astro-ph.CO2019

Partitioning the universe into gravitational basins using the cosmic velocity field

A. Dupuy, H. M. Courtois, F. Dupont +8

This letter presents a new approach using the cosmic peculiar velocity field to characterize the morphology and size of large scale structures in the local Universe. The algorithm…

astro-ph.CO2019

Cosmicflows-3: Cosmography of the Local Void

R Brent Tully, Daniel Pomarede, Romain Graziani +3

Cosmicflows-3 distances and inferred peculiar velocities of galaxies have permitted the reconstruction of the structure of over and under densities within the volume extending to 0…

astro-ph.CO201990 cited

The peculiar velocity field up to by forward-modeling Cosmicflows-3 data

R. Graziani, H. M. Courtois, G. Lavaux +4

A hierarchical Bayesian model is applied to the Cosmicflows-3 catalog of galaxy distances in order to derive the peculiar velocity field and distribution of matter within $z \sim 0…