activity
19942017
most citedDetecting filamentary pattern in the cosmic web: a catalogue of filaments for the SDSS

293 citations · 814 across the 19 of their papers we have counts for

collaborators

20 papers

astro-ph.EP2017★ 30 cited

KIC 8462852: Will the Trojans return in 2021?

Fernando J. Ballesteros, Pablo Arnalte-Mur, Alberto Fernandez-Soto +1

KIC 8462852 stood out among more than 100,000 stars in the Kepler catalogue because of the strange features of its light curve: a wide, asymmetric dimming taking up to 15 per cent…

astro-ph.CO2017★ 32 cited

The best fit for the observed galaxy Counts-in-Cell distribution function

Ll. Hurtado-Gil, V. J. Martínez, P. Arnalte-Mur +3

The Sloan Digital Sky Survey (SDSS) is the first dense redshift survey encompassing a volume large enough to find the best analytic probability density function that fits the galax…

astro-ph.CO2015★ 13 cited

Shell-like structures in our cosmic neighbourhood

M. Einasto, P. Heinämäki, L. J. Liivamägi +6

Signatures of the processes in the early Universe are imprinted in the cosmic web. Some of them may define shell-like structures characterised by typical scales. We search for shel…

astro-ph.CO2013★ 293 cited

Detecting filamentary pattern in the cosmic web: a catalogue of filaments for the SDSS

E. Tempel, R. S. Stoica, V. J. Martinez +3

The main feature of the spatial large-scale galaxy distribution is its intricate network of galaxy filaments. This network is spanned by the galaxy locations that can be interprete…

astro-ph.CO2012★ 52 cited

Multimodality of rich clusters from the SDSS DR8 within the supercluster-void network

M. Einasto, L. J. Liivamagi, E. Tempel +9

We study the relations between the multimodality of galaxy clusters drawn from the SDSS DR8 and the environment where they reside. As cluster environment we consider the global lum…

astro-ph.CO2012★ 77 cited

Multimodality in galaxy clusters from SDSS DR8: substructure and velocity distribution

M. Einasto, J. Vennik, P. Nurmi +8

We search for the presence of substructure, a non-Gaussian, asymmetrical velocity distribution of galaxies, and large peculiar velocities of the main galaxies in galaxy clusters wi…