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researcher

S. Morrison

4 papers hereh-index 10379 citations23 works total

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

author position
  • first author1
  • middle author2
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP4
same name
  • S. Morrison — 9 papers, h 22
  • S. Morrison — 6 papers, h 11
  • S. Morrison — 3 papers, h 6
  • S. Morrison — 2 papers, h 3
  • S. Morrison — 1 paper, h 1
  • S. Morrison — 1 paper

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
20162020
most citedALMA 1.3 Millimeter Map of the HD 95086 System

41 citations · 55 across the 2 of their papers we have counts for

collaborators

4 papers

astro-ph.EP2020

Forming Diverse Super-Earth Systems in Situ

Mariah G. MacDonald, Rebekah I. Dawson, Sarah J. Morrison +2

Super-Earths and mini-Neptunes exhibit great diversity in their compositional and orbital properties. Their bulk densities span a large range, from those dense enough to be purely…

astro-ph.EP2019★ 14 cited

Debris Disks in Multi-Planet Systems: Are Our Inferences Compromised by Unseen Planets?

Jiayin Dong, Rebekah I. Dawson, Andrew Shannon +1

Resolved debris disk features (e.g., warps, offsets, edges and gaps, azimuthal asymmetries, radially thickened rings, scale heights) contain valuable information about the underlyi…

astro-ph.EP2017★ 41 cited

ALMA 1.3 Millimeter Map of the HD 95086 System

Kate Y. L. Su, Meredith A. Macgregor, Mark Booth +11

Planets and minor bodies such as asteroids, Kuiper-belt objects and comets are integral components of a planetary system. Interactions among them leave clues about the formation pr…

astro-ph.EP2016

Orbital Stability of Multi-Planet Systems: Behavior at High Masses

Sarah J. Morrison, Kaitlin M. Kratter

In the coming years, high contrast imaging surveys are expected to reveal the characteristics of the population of wide-orbit, massive, exoplanets. To date, a handful of wide plane…

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