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E. Saar

78 papers hereh-index 435.8k citations180 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author39
  • last author18

Across the 58 of 78 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO42
  • astro-ph33
  • astro-ph.GA2
  • stat.AP1
same name
  • E. Saar — 1 paper

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19942022
most citedPlanck Early Results VIII: The all-sky Early Sunyaev-Zeldovich cluster sample

413 citations · 4.2k across the 78 of their papers we have counts for

collaborators
Showing 2016Show all

4 papers · 1 filter

astro-ph.GA2016★ 54 cited

Alignment of galaxies relative to their local environment in SDSS-DR8

A. Hirv, J. Pelt, E. Saar +4

We study the alignment of galaxies relative to their local environment in SDSS-DR8 and, using these data, we discuss evolution scenarios for different types of galaxies. We defined…

astro-ph.CO2016★ 41 cited

Sloan Great Wall as a complex of superclusters with collapsing cores

Maret Einasto, Heidi Lietzen, Mirt Gramann +6

In the cosmic web, galaxy superclusters or their high-density cores are the largest objects that may collapse at present or during the future evolution. We study the dynamical stat…

astro-ph.CO2016

Bisous model - detecting filamentary patterns in point processes

E. Tempel, R. S. Stoica, R. Kipper +1

The cosmic web is a highly complex geometrical pattern, with galaxy clusters at the intersection of filaments and filaments at the intersection of walls. Identifying and describing…

astro-ph.CO2016★ 44 cited

Discovery of a massive supercluster system at z∼0.47

H. Lietzen, E. Tempel, L. J. Liivamägi +6

Superclusters are the largest relatively isolated systems in the cosmic web. Using the SDSS BOSS survey we search for the largest superclusters in the redshift range 0.43<z<0.71.…

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