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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.COShow all

3 papers · 1 filter

astro-ph.CO2023★ 11 cited

CONCERTO: Extracting the power spectrum of the [C II ] emission line

M. Van Cuyck, N. Ponthieu, G. Lagache +21

CONCERTO is the first experiment to perform a [CII] line intensity mapping survey to target z>5.2. Measuring the [CII] power spectrum allows us to study the role of dusty star-fo…

astro-ph.CO2022

CONCERTO: Simulating the CO, [CII], and [CI] line emission of galaxies in a 117 deg2 field and the impact of field-to-field variance

A. Gkogkou, M. Béthermin, G. Lagache +29

In the submm regime, spectral line scans and line intensity mapping (LIM) are new promising probes for the cold gas content and star formation rate of galaxies across cosmic time.…

astro-ph.CO2013★ 125 cited

Evolution of the mass, size, and star formation rate in high-redshift merging galaxies MIRAGE - A new sample of simulations with detailed stellar feedback

V. Perret, F. Renaud, B. Epinat +5

We aim at addressing the questions related to galaxy mass assembly through major and minor wet merging processes in the redshift range 1<z<2. A consequent fraction of Milky Way lik…

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