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researcher

D. Johnstone

37 papers hereh-index 292.3k citations87 works total

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

author position
  • middle author25
  • last author2

Across the 27 of 37 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA18
  • astro-ph.SR16
  • astro-ph2
  • astro-ph.EP1
same name
  • D. Johnstone — 195 papers, h 52
  • D. Johnstone — 19 papers, h 15
  • D. Johnstone — 15 papers, h 7
  • D. Johnstone — 15 papers, h 5
  • D. Johnstone — 14 papers, h 14
  • D. Johnstone — 7 papers, h 22

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 citedWater in star-forming regions with Herschel (WISH): II. Evolution of 557 GHz 110-101 emission in low-mass protostars

273 citations · 1.7k across the 37 of their papers we have counts for

collaborators
Showing 2013Show all

3 papers · 1 filter

astro-ph.GA2013★ 76 cited

Water in star-forming regions with Herschel (WISH). IV. A survey of low-J H2O line profiles toward high-mass protostars

Floris van der Tak, Luis Chavarria, Fabrice Herpin +4

To understand the origin of water line emission and absorption during high-mass star formation, we decompose high-resolution Herschel-HIFI line spectra toward 19 high-mass star-for…

astro-ph.GA2013★ 131 cited

The Herschel and JCMT Gould Belt Surveys: Constraining Dust Properties in the Perseus B1 Clump with PACS, SPIRE, and SCUBA-2

S. I. Sadavoy, J. Di Francesco, D. Johnstone +27

We present Herschel observations from the Herschel Gould Belt Survey and SCUBA-2 science verification observations from the JCMT Gould Belt Survey of the B1 clump in the Perseus mo…

astro-ph.GA2013★ 47 cited

Herschel-HIFI observations of high-J CO and isotopologues in star-forming regions: from low- to high-mass

I. San Jose-Garcia, J. C. Mottram, L. E. Kristensen +9

Context; Our understanding of the star formation process has traditionally been confined to certain mass or luminosity boundaries because most studies focus only on low-, intermedi…

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