activity
20062026
most citedSuperclusters of galaxies from the 2dF redshift survey. I. The catalogue

104 citations · 351 across the 15 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

11 papers · 1 filter

astro-ph.CO2026

J-PAS & FLAMINGO: Cosmic voids and void galaxies in the gravitational landscape of photometric surveys

J. A. Mansour, B. McCarthy, L. J. Liivamägi +34

Photometric surveys offer a powerful way to map the large-scale structure of the Universe, but their redshift errors complicate the identification of cosmic voids, challenging stud…

astro-ph.CO2023

Galaxy groups and clusters and their brightest galaxies within the cosmic web

Maret Einasto, Jaan Einasto, Peeter Tenjes +5

Our aim is to combine data on single galaxies, galaxy groups, their BGGs, and their location in the cosmic web, to determine classes of groups, and to obtain a better understanding…

astro-ph.CO2023★ 5 cited

Evolution of matter and galaxy clustering in cosmological hydrodynamical simulations

Jaan Einasto, Gert Hütsi, Lauri-Juhan Liivamägi +4

We quantify the evolution of matter and galaxy clustering in cosmological hydrodynamical simulations via correlation and bias functions of matter and galaxies. We use simulations T…

astro-ph.CO2022★ 14 cited

The evolution of high-density cores of the BOSS Great Wall superclusters

Maret Einasto, Peeter Tenjes, Mirt Gramann +6

High-density cores (HDCs) of galaxy superclusters that embed rich clusters and groups of galaxies are the earliest large objects to form in the cosmic web, and the largest objects…

astro-ph.CO2021★ 8 cited

The shape distribution of superclusters in SDSS DR 12

Satadru Bag, Lauri Juhan Liivamägi, Maret Einasto

Galaxy superclusters, the largest galaxy structures in the cosmic web, are formed due to the gravitational collapse (although they are not usually gravitationally bound). Their geo…

astro-ph.CO2020

Evolution of skewness and kurtosis of cosmic density fields

Jaan Einasto, Anatoly Klypin, Gert Hütsi +2

Methods. We perform numerical simulations of the evolution of the cosmic web for the conventional LCDM model. The simulations cover a wide range of box sizes L = 256 - 4000 Mpc/h,…