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researcher

M. Rainer

101 papers hereh-index 326.4k citations194 works total

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

author position
  • first author2
  • middle author78
  • last author2

Across the 82 of 101 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP48
  • astro-ph.SR40
  • astro-ph.IM7
  • astro-ph.GA3
  • physics.optics2
  • astro-ph1
same name
  • M. Rainer — 39 papers, h 17
  • M. Rainer — 27 papers, h 11
  • M. Rainer — 10 papers, h 8
  • M. Rainer — 9 papers
  • M. Rainer — 1 paper, h 0
  • M. Rainer — 1 paper, h 0

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
20072026
most citedThe GAPS Programme with HARPS-N@TNG XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets

358 citations · 4k across the 99 of their papers we have counts for

collaborators
Showing 2013Show all

3 papers · 1 filter

astro-ph.SR2013★ 139 cited

The GAPS programme with HARPS-N at TNG. I: Observations of the Rossiter-McLaughlin effect and characterisation of the transiting system Qatar-1

E. Covino, M. Esposito, M. Barbieri +67

A long-term multi-purpose observational programme has started with HARPS-N@TNG aimed to characterise the global architectural properties of exoplanetary systems. In this first pape…

astro-ph.EP2013★ 46 cited

The GAPS Programme with HARPS-N@TNG II: No giant planets around the metal-poor star HIP 11952

S. Desidera, A. Sozzetti, A. S. Bonomo +37

In the context of the program Global Architecture of Planetary Systems (GAPS), we have performed radial velocity monitoring of the metal-poor star HIP 11952 on 35 nights over about…

astro-ph.SR2013★ 5 cited

Understanding the dynamical structure of pulsating stars: The Baade-Wesselink projection factor of the delta Scuti stars AI Vel and beta Cas

G. Guiglion, N. Nardetto, P. Mathias +6

Aims. The Baade-Wesselink method of distance determination is based on the oscillations of pulsating stars. The key parameter of this method is the projection factor used to conver…

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