activity
20062022
most cited4MOST: Project overview and information for the First Call for Proposals

311 citations · 1.4k across the 37 of their papers we have counts for

collaborators
Showing 2018Show all

8 papers · 1 filter

astro-ph.CO2018

To be or not to be: hot WHIM absorption in the blazar PKS 2155-304 sight line?

J. Nevalainen, E. Tempel, J. Ahoranta +8

The cosmological missing baryons at z<1 most likely hide in the hot (T K) phase of the Warm Hot Intergalactic Medium (WHIM). While the hot WHIM is hard to detect d…

astro-ph.CO2018

Supercluster A2142 and collapse in action - infalling and merging groups and galaxy transformations

Maret Einasto, Mirt Gramann, Changbom Park +8

We study the dynamical state and properties of galaxies and groups in the supercluster SClA2142 that has a collapsing core, to understand its possible formation and evolution. We f…

astro-ph.GA2018

A method to calculate gravitational accelerations within discrete localised regions in the Milky Way

Rain Kipper, Elmo Tempel, Peeter Tenjes

We present a method to calculate gravitational potential gradients within regions containing few tens of thousands stars with known phase space coordinates. The central idea of the…

astro-ph.CO2018

Bayesian group finder based on marked point processes. Method and feasibility study using the 2MRS data set

Elmo Tempel, Maarja Kruuse, Rain Kipper +3

Galaxy groups and clusters are formidable cosmological probes. They permit the studying of the environmental effects on galaxy formation. A reliable detection of galaxy groups is a…

astro-ph.CO2018

Galaxy Cluster Mass Reconstruction Project - IV. Understanding the effects of imperfect membership on cluster mass estimation

R. Wojtak, L. Old, G. A. Mamon +17

The primary difficulty in measuring dynamical masses of galaxy clusters from galaxy data lies in the separation between true cluster members from interloping galaxies along the lin…

astro-ph.GA2018

The shape alignment of satellite galaxies in galaxy pairs in SDSS

Peng Wang, Quan Guo, Noam I. Libeskind +3

It has been shown, both in simulations and observationally, that the tidal field of a large galaxy can torque its satellites such that the major axis of satellite galaxies points t…