Ultraviolet dust attenuation in star-forming galaxies – II. Calibrating the A(UV) versus LTIR/LUV relation
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NGC 4370: a case study for testing our ability to infer dust distribution and mass in nearby galaxiesThe GALEX Ultraviolet Virgo Cluster Survey (GUViCS)The WiggleZ Dark Energy Survey: star formation in UV-luminous galaxies from their luminosity functionsComparison of star formation rates from Hα and infrared luminosity as seen byHerschelThe VIMOS VLT Deep SurveyFar-infrared colours of nearby late-type galaxies in the Herschel Reference SurveyCold gas properties of the Herschel Reference Survey II. Molecular and total gas scaling relationsH-ATLAS/GAMA: the nature and characteristics of optically red galaxies detected at submillimetre wavelengthsThe Dawn of the Red: star formation histories of group galaxies over the past 5 billion yearsEncoding of the infrared excess in theNUVrKcolor diagram for star-forming galaxiesDust attenuation up to z ≃ 2 in the AKARI North Ecliptic Pole Deep Field
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Ultraviolet dust attenuation in star-forming galaxies – II. Calibrating the A(UV) versus LTIR/LUV relation
description
im Mai 2008 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована в травні 2008
@uk
name
Ultraviolet dust attenuation in star-forming galaxies – II. Calibrating the A
@nl
Ultraviolet dust attenuation i ...... A(UV) versus LTIR/LUV relation
@en
type
label
Ultraviolet dust attenuation in star-forming galaxies – II. Calibrating the A
@nl
Ultraviolet dust attenuation i ...... A(UV) versus LTIR/LUV relation
@en
prefLabel
Ultraviolet dust attenuation in star-forming galaxies – II. Calibrating the A
@nl
Ultraviolet dust attenuation i ...... A(UV) versus LTIR/LUV relation
@en
P2860
P50
P1476
Ultraviolet dust attenuation i ...... A(UV) versus LTIR/LUV relation
@en
P2093
G. Gavazzi
R. Decarli
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P304
P356
10.1111/J.1365-2966.2008.13118.X
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P577
2008-05-01T00:00:00Z
P818
P819
2008MNRAS.386.1157C