activity
20062025
most citedTracing the cosmic web

361 citations · 4k across the 107 of their papers we have counts for

collaborators

107 papers

astro-ph.CO2025

TOPz: Photometric redshifts using template fitting applied to the GAMA survey

E. Tempel, J. Laur, Z. R. Jones +7

Context. Accurate photometric redshift estimation is crucial for cosmological and galaxy evolution studies, especially with the advent of large-scale photometric surveys. Aims. We…

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★ 1 cited

Identification of Superclusters and their Properties in the Sloan Digital Sky Survey Using WHL Cluster Catalog

Shishir Sankhyayan, Joydeep Bagchi, Elmo Tempel +6

Superclusters are the largest massive structures in the cosmic web on tens to hundreds of megaparsecs (Mpc) scales. They are the largest assembly of galaxy clusters in the Universe…

astro-ph.CO2023★ 3 cited

Statistically bias-minimized peculiar velocity catalogs from Gibbs point processes and Bayesian inference

Jenny G. Sorce, Radu S. Stoica, Elmo Tempel

Galaxy peculiar velocities are excellent cosmological probes provided that biases inherent to their measurements are contained before any study. This paper proposes a new algorithm…

astro-ph.GA2023

Kinematics of the Local Group gas and galaxies in the Hestia simulations

Luis Biaus, Sebastián E. Nuza, Cecilia Scannapieco

The Local Group (LG) consists of two giant spiral galaxies, the Milky Way (MW) and Andromeda (M31), and several smaller galaxies. The MW and M31 are approaching each other at a rad…

astro-ph.CO2023★ 10 cited

Cosmic metal invaders: Intergalactic OVII as a tracer of the warm-hot intergalactic medium within cosmic filaments in the EAGLE simulation

T. Tuominen, J. Nevalainen, P. Heinämäki +5

The current observational status of the hot (log T(K) > 5.5) warm-hot intergalactic medium (WHIM) remains incomplete. While recent observations from stacking large numbers of Cosmi…