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S. Muller

86 papers hereh-index 345.7k citations161 works total

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

author position
  • first author13
  • middle author55
  • last author4

Across the 72 of 86 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA51
  • astro-ph11
  • astro-ph.CO11
  • astro-ph.SR8
  • astro-ph.IM3
  • astro-ph.HE2
same name
  • S. Muller — 23 papers, h 13
  • S. Muller — 20 papers, h 24
  • S. Muller — 19 papers, h 4
  • S. Muller — 10 papers, h 7
  • S. Muller — 8 papers, h 4
  • S. Muller — 7 papers, h 19

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
20022023
most citedUVMULTIFIT: A versatile tool for fitting astronomical radio interferometric data

190 citations · 3.7k across the 86 of their papers we have counts for

collaborators
Showing 2012Show all

3 papers · 1 filter

astro-ph.CO2012★ 124 cited

A precise and accurate determination of the cosmic microwave background temperature at z=0.89

S. Muller, A. Beelen, J. H. Black +6

According to the Big Bang theory and as a consequence of adiabatic expansion of the Universe, the temperature of the cosmic microwave background (CMB) increases linearly with redsh…

astro-ph.CO2012★ 11 cited

Molecular gas and dust in the highly magnified z = 2.8 galaxy behind the Bullet Cluster

Daniel Johansson, Cathy Horellou, Omar Lopez-Cruz +8

The gravitational magnification provided by massive galaxy clusters makes it possible to probe the physical conditions in distant galaxies that are of lower luminosity than those i…

astro-ph.GA2012★ 67 cited

Winds of change - a molecular outflow in NGC 1377? The anatomy of an extreme FIR-excess galaxy

S. Aalto, S. Muller, K. Sakamoto +3

We use high (0."65 x 0."52,(65x52pc)) resolution SubMillimeter Array (SMA) observations to image the CO and 13CO 2-1 line emission of the extreme FIR-excess galaxy NGC 1377. We fin…

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