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researcher

G. Duchêne

40 papers hereh-index 271.8k citations58 works total

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

author position
  • first author3
  • middle author24
  • last author1

Across the 28 of 40 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR20
  • astro-ph8
  • astro-ph.EP8
  • astro-ph.GA4
same name
  • G. Duchêne — 127 papers, h 58
  • G. Duchêne — 70 papers, h 35
  • G. Duchêne — 12 papers, h 4
  • G. Duchêne — 10 papers, h 12
  • G. Duchêne — 5 papers, h 5
  • G. Duchêne — 4 papers, 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
20042026
most citedProbing dust grain evolution in IM Lupi's circumstellar disc. Multi-wavelength observations and modelling of the dust disc

193 citations · 1.8k across the 40 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2024★ 12 cited

Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Our Galaxy

Pamela Klaassen, Alessio Traficante, Maria T. Beltrán +38

As we learn more about the multi-scale interstellar medium (ISM) of our Galaxy, we develop a greater understanding for the complex relationships between the large-scale diffuse gas…

astro-ph.GA2013★ 128 cited

GASPS - a Herschel survey of gas and dust in Protoplanetary Disks: Summary and Initial Statistics

W. R. F. Dent, W. F. Thi, I. Kamp +47

GASPS is a far-infrared line and continuum survey of protoplanetary and young debris disks using PACS on the Herschel Space Observatory. The survey includes [OI] at 63 microns, as…

astro-ph.GA2012★ 76 cited

Spectroscopy of brown dwarf candidates in IC 348 and the determination of its substellar IMF down to planetary masses

C. Alves de Oliveira, E. Moraux, J. Bouvier +4

Context. Brown dwarfs represent a sizable fraction of the stellar content of our Galaxy and populate the transition between the stellar and planetary mass regime. There is however…

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