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researcher

S. Gottlöber

110 papers hereh-index 8526 citations78 works total

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

author position
  • sole author1
  • first author4
  • middle author79
  • last author22

Across the 106 of 110 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO65
  • astro-ph.GA25
  • astro-ph18
  • astro-ph.HE1
  • astro-ph.IM1
same name
  • S. Gottlöber — 8 papers, h 23
  • S. Gottlöber — 6 papers, h 11
  • S. Gottlöber — 3 papers, h 4

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
19952026
most citedA Dynamical Classification of the Cosmic Web

292 citations · 5.5k across the 107 of their papers we have counts for

collaborators
Showing 2016Show all

4 papers · 1 filter

astro-ph.GA2016★ 33 cited

Constraining the mass of the Local Group

Edoardo Carlesi, Yehuda Hoffman, Jenny G. Sorce +1

The mass of the Local Group (LG) is a crucial parameter for galaxy formation theories. However, its observational determination is challenging - its mass budget is dominated by dar…

astro-ph.CO2016★ 15 cited

Galaxy Three-Point Correlation Functions and Halo/Subhalo Models

Hong Guo, Zheng Zheng, Peter S. Behroozi +9

We present the measurements of the luminosity-dependent redshift-space three-point correlation functions (3PCFs) for the Sloan Digital Sky Survey (SDSS) DR7 Main galaxy sample. We…

astro-ph.CO2016★ 36 cited

How did the Virgo cluster form?

Jenny G. Sorce, Stefan Gottloeber, Yehuda Hoffman +1

While the Virgo cluster is the nearest galaxy cluster and therefore the best observed one, little is known about its formation history. In this paper, a set of cosmological simulat…

astro-ph.GA2016★ 11 cited

The tangential velocity of M31: CLUES from constrained simulations

Edoardo Carlesi, Yehuda Hoffman, Jenny G. Sorce +4

Determining the precise value of the tangential component of the velocity of M31 is a non trivial astrophysical issue, that relies on complicated modeling. This has recently lead t…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.