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researcher

S. Hansen

43 papers hereh-index 314.8k citations122 works total

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

author position
  • sole author9
  • first author8
  • middle author13
  • last author13

Across the 43 of 43 papers where every author was matched, so the position is known.

fields
  • astro-ph24
  • astro-ph.CO10
  • astro-ph.GA4
  • hep-ph2
  • gr-qc1
  • math.GM1
same name
  • S. Hansen — 13 papers, h 10
  • S. Hansen — 8 papers, h 13
  • S. Hansen — 5 papers, h 7
  • S. Hansen — 5 papers, h 16
  • S. Hansen — 4 papers, h 33
  • S. Hansen — 3 papers, h 5

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
20012026
most citedA universal density slope - velocity anisotropy relation for relaxed structures

201 citations · 596 across the 29 of their papers we have counts for

collaborators
Showing 2003 · astro-phShow all

4 papers · 2 filters

astro-ph2003

Galactic hydraulic drop?

Steen H. Hansen

Galaxies and galaxy clusters are observed to have a rather non-trivial radial behaviour. The observations show that the radial profiles change from one power-law profile near the c…

astro-ph2003

Extraction of cluster parameters from Sunyaev-Zeldovich effect observations with simulated annealing optimization

Steen H. Hansen

We present a user-friendly tool for the analysis of data from Sunyaev-Zeldovich effect observations. The tool is based on the stochastic method of simulated annealing, and allows t…

astro-ph2003

Constraining the helium abundance with CMB

Roberto Trotta, Steen H. Hansen

We consider for the first time the ability of present-day cosmic microwave background (CMB) anisotropies data to determine the primordial helium mass fraction, Y_p. We find that CM…

astro-ph2003

The origin of cores and density profiles of gaseous baryonic structures

Steen H. Hansen, Joachim Stadel

We study the origin of cores and density profiles of gaseous baryonic structures in cosmology. By treating the baryons as a viscous gas, we find that both spheres and disks are pos…

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