about
The dust morphology of the elliptical Galaxy M 86 with SPIREDiscovery of a galaxy cluster with a violently starbursting core at z = 2.506The Herschel Virgo Cluster Survey - VIII. The Bright Galaxy SampleProbing the Baryon Cycle of Galaxies with SPICA Mid- and Far-Infrared ObservationsWelcome to the Twilight Zone: The Mid-infrared Properties of Post-starburst GalaxiesDust spectral energy distributions of nearby galaxies: an insight from the Herschel Reference SurveyPACS photometry of the Herschel Reference Survey – far-infrared/submillimetre colours as tracers of dust properties in nearby galaxiesThe Herschel Virgo Cluster Survey XV. Planck submillimetre sources in the Virgo ClusterThe Herschel Virgo Cluster Survey – XIV. Transition-type dwarf galaxies in the Virgo clusterSubmillimetre photometry of 323 nearby galaxies from the Herschel Reference Survey (Corrigendum)The Herschel Fornax Cluster Survey – I. The bright galaxy sampleThe Herschel Virgo Cluster Survey – XII. FIR properties of optically selected Virgo cluster galaxiesThe Herschel Virgo Cluster Survey XI. Environmental effects on molecular gas and dust in spiral disksSubmillimetre photometry of 323 nearby galaxies from the Herschel Reference SurveyThe Herschel reference survey: dust in early-type galaxies and across the Hubble sequenceThe dust scaling relations of the Herschel Reference SurveyFIR colours and SEDs of nearby galaxies observed with HerschelA molecular gas-rich GRB host galaxy at the peak of cosmic star formationTracing the Evolution of Dust Obscured Star Formation and Accretion Back to the Reionisation Epoch with SPICAThe physical properties ofSpitzer/IRS galaxies derived from their UV to 22μm spectral energy distributionStudying the evolution of galaxies in compact groups over the past 3 Gyr – II. The importance of environment in the suppression of star formationThe imprint of rapid star formation quenching on the spectral energy distributions of galaxiesStudying the evolution of galaxies in compact groups over the past 3 Gyr – I. Nuclear activityConstraining the properties of AGN host galaxies with spectral energy distribution modellingThe Herschel Virgo Cluster Survey XIX. Physical properties of low luminosity FIR sources at z < 0.5Can dust emission Be used to estimate the mass of the interstellar medium in Galaxies--A pilot project with the Herschel reference surveyFar-infrared colours of nearby late-type galaxies in the Herschel Reference SurveyObservational evidence of a slow downfall of star formation efficiency in massive galaxies during the past 10 GyrInfrared color selection of massive galaxies at z > 3Revealing the Environmental Dependence of Molecular Gas Content in a Distant X-Ray Cluster at z = 2.51An enhanced fraction of starbursting galaxies among high Eddington ratio AGNsHerschel deep far-infrared counts through Abell 2218 cluster-lensThe ASTRODEEP Frontier Fields cataloguesThe ASTRODEEP Frontier Fields cataloguesDust attenuation up to z ≃ 2 in the AKARI North Ecliptic Pole Deep FieldGalaxy Evolution Studies with the SPace IR Telescope for Cosmology and Astrophysics (SPICA): The Power of IR SpectroscopySPICA and the Chemical Evolution of Galaxies: The Rise of Metals and DustRevealing the cold dust in low-metallicity environments (Corrigendum)An Overview of the Dwarf Galaxy Survey (PASP, 125, 600, [2013])—CorrigendumThe Herschel Exploitation of Local Galaxy Andromeda (HELGA) . IV. Dust scaling relations at sub-kpc resolution
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description
Frans onderzoekster
@nl
French astrophysicist
@en
astrofísica francesa
@es
astrophysicienne française
@fr
name
Laure Ciesla
@ast
Laure Ciesla
@en
Laure Ciesla
@es
Laure Ciesla
@fr
Laure Ciesla
@nl
Laure Ciesla
@sl
type
label
Laure Ciesla
@ast
Laure Ciesla
@en
Laure Ciesla
@es
Laure Ciesla
@fr
Laure Ciesla
@nl
Laure Ciesla
@sl
prefLabel
Laure Ciesla
@ast
Laure Ciesla
@en
Laure Ciesla
@es
Laure Ciesla
@fr
Laure Ciesla
@nl
Laure Ciesla
@sl