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researcher

M. Gunther

44 papers hereh-index 323 citations19 works total

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

author position
  • middle author39
  • last author1

Across the 40 of 44 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP38
  • astro-ph.SR5
  • astro-ph.IM1
same name
  • M. Gunther — 8 papers, h 20
  • M. Gunther — 8 papers, h 10
  • M. Gunther — 1 paper, h 1
  • M. Gunther — 1 paper, h 1

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
20202026
most citedSix transiting planets and a chain of Laplace resonances in TOI-178

195 citations · 547 across the 40 of their papers we have counts for

collaborators
Showing 2021Show all

4 papers · 1 filter

astro-ph.EP2021

A large sub-Neptune transiting the thick-disk M4V TOI-2406

R. D. Wells, B. V. Rackham, N. Schanche +71

Large sub-Neptunes are uncommon around the coolest stars in the Galaxy and are rarer still around those that are metal-poor. However, owing to the large planet-to-star radius ratio…

astro-ph.EP2021★ 195 cited

Six transiting planets and a chain of Laplace resonances in TOI-178

A. Leleu, Y. Alibert, N. C. Hara +152

Determining the architecture of multi-planetary systems is one of the cornerstones of understanding planet formation and evolution. Resonant systems are especially important as the…

astro-ph.SR2021

KIC 2852961 -- a superflaring red monster in the Kepler field

Zs. Kővári, K. Oláh, M. N. Günther +3

Superflares on giant stars have up to 100,000 times more energy than the high energy solar flares. However, it is disputed, whether scaling up a solar-type dynamo could explain suc…

astro-ph.EP2021★ 18 cited

NGTS-14Ab: a Neptune-sized transiting planet in the desert

A. M. S. Smith, J. S. Acton, D. R. Anderson +35

Context: The sub-Jovian or Neptunian desert is a previously-identified region of parameter space where there is a relative dearth of intermediate-mass planets at short orbital peri…

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