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researcher

A. Müller

17 papers hereh-index 6541 citations11 works total

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

author position
  • first author1
  • middle author9
  • last author4

Across the 14 of 17 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP9
  • astro-ph.SR6
  • astro-ph2
same name
  • A. Müller — 35 papers, h 35
  • A. Müller — 12 papers, h 6
  • A. Müller — 11 papers, h 11
  • A. Müller — 7 papers, h 23
  • A. Müller — 7 papers, h 10
  • A. Müller — 6 papers, h 30

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
20052020
most citedThe SPHERE infrared survey for exoplanets (SHINE). III. The demographics of young giant exoplanets below 300 au with SPHERE

230 citations · 1.2k across the 17 of their papers we have counts for

collaborators
Showing 2020Show all

3 papers · 1 filter

astro-ph.EP2020★ 27 cited

The search for disks or planetary objects around directly imaged companions: A candidate around DH Tau B

C. Lazzoni, A. Zurlo, S. Desidera +45

In recent decades, thousands of substellar companions have been discovered with both indirect and direct methods of detection. In this paper, we focus our attention on substellar c…

astro-ph.EP2020★ 230 cited

The SPHERE infrared survey for exoplanets (SHINE). III. The demographics of young giant exoplanets below 300 au with SPHERE

A. Vigan, C. Fontanive, M. Meyer +108

The SHINE project is a 500-star survey performed with SPHERE on the VLT for the purpose of directly detecting new substellar companions and understanding their formation and early…

astro-ph.EP2020★ 40 cited

ISPY -- NACO Imaging Survey for Planets around Young stars: Survey description and results from the first 2.5 years of observations

R. Launhardt, Th. Henning, A. Quirrenbach +21

The occurrence rate of long-period giant planets around young stars is highly uncertain since it is not only governed by the protoplanetary disc structure and planet formation proc…

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