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researcher

J. Lambert

14 papers hereh-index 11634 citations23 works total

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

author position
  • middle author9
  • last author3

Across the 12 of 14 papers where every author was matched, so the position is known.

fields
  • astro-ph4
  • astro-ph.CO3
  • astro-ph.GA3
  • astro-ph.IM3
  • astro-ph.EP1
same name
  • J. Lambert — 5 papers, h 3
  • J. Lambert — 5 papers, h 4
  • J. Lambert — 5 papers, h 3
  • J. Lambert — 4 papers, h 3
  • J. Lambert — 3 papers, h 3
  • J. Lambert — 2 papers, h 19

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
19972023
most citedCan bars be destroyed by a central mass concentration? I. Simulations

171 citations · 762 across the 14 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2022★ 21 cited

Supervised machine learning on Galactic filaments Revealing the filamentary structure of the Galactic interstellar medium

A. Zavagno, F. -X. Dupé, S. Bensaid +11

Context. Filaments are ubiquitous in the Galaxy, and they host star formation. Detecting them in a reliable way is therefore key towards our understanding of the star formation pro…

astro-ph.GA2022★ 56 cited

CONCERTO: High-fidelity simulation of millimeter line emissions of galaxies and [CII] intensity mapping

M. Bethermin, A. Gkogkou, M. Van Cuyck +27

The intensity mapping of the [CII] 158um line redshifted to the sub-mm window is a promising probe of the z>4 star formation and its spatial distribution into the large-scale struc…

astro-ph.GA2016★ 122 cited

Forming disk galaxies in wet major mergers. I. Three fiducial examples

E. Athanassoula, S. A. Rodionov, N. Peschken +1

Using three fiducial Nbody+SPH simulations, we follow the merging of two disk galaxies with a hot gaseous halo component each, and examine whether the merger remnant can be a spira…

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