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Probing the cold and warm molecular gas in the Whirlpool Galaxy : Herschel SPIRE-FTS observations of the central region of M51 (NGC 5194)
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The Herschel exploitation of local galaxy Andromeda (HELGA), VII : a SKIRT radiative transfer model and insights on dust heating
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The Herschel Virgo Cluster Survey, XX : dust and gas in the foreground Galactic cirrus
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The selective effect of environment on the atomic and molecular gas-to-dust ratio of nearby galaxies in the Herschel Reference Survey
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The bolometric and UV attenuation in normal spiral galaxies of the Herschel Reference Survey
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The imprint of rapid star formation quenching on the spectral energy distributions of galaxies
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The spatially resolved correlation between [NII] 205 µm line emission and the 24 µm continuum in nearby galaxies
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Hα imaging of the Herschel Reference Survey : the star formation properties of a volume-limited, K-band-selected sample of nearby late-type galaxies
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The relationship between polycyclic aromatic hydrocarbon emission and far-infrared dust emission from NGC 2403 and M83
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NGC 4370 : a case study for testing our ability to infer dust distribution and mass in nearby galaxies
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Linking dust emission to fundamental properties in galaxies : the low-metallicity picture
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The identification of dust heating mechanisms in nearby galaxies using Herschel 160/250 and 250/350 µm surface brightness ratios
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Insights into gas heating and cooling in the disc of NGC 891 from Herschel far-infrared spectroscopy
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The Herschel Dwarf Galaxy Survey, I : properties of the low-metallicity ISM from PACS spectroscopy
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The Herschel exploitation of local galaxy Andromeda (HELGA), VI : the distribution and properties of molecular cloud associations in M31
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Spatially resolved physical conditions of molecular gas and potential star formation tracers in M83, revealed by the Herschel SPIRE FTS
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The Herschel Virgo Cluster survey, XVIII : star-forming dwarf galaxies in a cluster environment
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The bivariate K-band-submillimetre luminosity functions of the local HRS galaxy sample
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Quantifying the heating sources for mid-infrared dust emissions in galaxies : the case of M 81
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The physical characteristics of the gas in the disk of Centaurus A using the Herschel Space Observatory