activity
19992023
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 24.3k across the 133 of their papers we have counts for

collaborators

133 papers

astro-ph.GA2023★ 1 cited

NIKA2 observations of starless cores in Taurus and Perseus

C. Kramer, R. Adam, P. Ade +49

Dusty starless cores play an important role in regulating the initial phases of the formation of stars and planets. In their interiors, dust grains coagulate and ice mantles form,…

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 . Measuring the [CII] power spectrum allows us to study the role of dusty star-fo…

astro-ph.GA2023★ 18 cited

NIKA2 Cosmological Legacy Survey: Survey Description and Galaxy Number Counts

L. Bing, M. Béthermin, G. Lagache +48

Aims. Deep millimeter surveys are necessary to probe the dust-obscured galaxies at high redshift. We conducted a large observing program at 1.2 and 2 mm with the NIKA2 camera insta…

astro-ph.CO2022

CONCERTO: Simulating the CO, [CII], and [CI] line emission of galaxies in a 117 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.GA2022★ 3 cited

Sub-GeV Dark Matter Searches with EDELWEISS: New results and prospects

H. Lattaud

The Edelweiss collaboration performs light Dark Matter (DM) particles searches with germanium bolometer collecting charge and phonon signals. Thanks to the Neganov-Trofimov-Luke (N…

astro-ph.CO2022★ 1 cited

Candidate cosmic filament in the GJ526 field, mapped with the NIKA2 camera

J. -F. Lestrade, F. -X. Desert, G. Lagache +44

Distinctive large-scale structures have been identified in the spatial distribution of optical galaxies up to redshift z ~ 1. In the more distant universe, the relationship between…