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researcher

Marshall C. Johnson

62 papers hereh-index 251.8k citations91 works total

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

author position
  • first author10
  • middle author38
  • last author1

Across the 49 of 62 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP49
  • astro-ph.SR9
  • astro-ph.GA2
  • astro-ph.IM1
  • cs.NI1
same name
  • Marshall C. Johnson — 7 papers, h 4
  • Marshall C. Johnson — 5 papers, h 3
  • Marshall C. Johnson — 5 papers, h 1
  • Marshall C. Johnson — 1 paper
  • Marshall C. Johnson — 1 paper, h 2
  • Marshall C. Johnson — 1 paper, h 2

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
20122024
most citedA giant planet undergoing extreme ultraviolet irradiation by its hot massive-star host

270 citations · 2.6k across the 61 of their papers we have counts for

collaborators
Showing 2024Show all

3 papers · 1 filter

astro-ph.EP2024

Mass determination of two Jupiter-sized planets orbiting slightly evolved stars: TOI-2420 b and TOI-2485 b

Ilaria Carleo, Oscar Barrágan, Carina M. Persson +67

Hot and warm Jupiters might have undergone the same formation and evolution path, but the two populations exhibit different distributions of orbital parameters, challenging our und…

astro-ph.EP2024

Trials and Tribulations in the Reanalysis of KELT-24 b: a Case Study for the Importance of Stellar Modeling

Mark R. Giovinazzi, Bryson Cale, Jason D. Eastman +21

We present a new analysis of the KELT-24 system, comprising a well-aligned hot Jupiter, KELT-24~b, and a bright (V=8.3), nearby (d=96.9 pc) F-type host star. KELT-24~b…

astro-ph.EP2024

Wide Binary Orbits are Preferentially Aligned with the Orbits of Small Planets, but Probably Not Hot Jupiters

Sam Christian, Andrew Vanderburg, Juliette Becker +28

Studying the relative orientations of the orbits of exoplanets and wide-orbiting binary companions (semimajor axis greater than 100 AU) can shed light on how planets form and evolv…

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