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http://hub.abes.fr/edp/periodical/aa/2011/volume_532/issue_2011/aa16447-11/authorship/5
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http://hub.abes.fr/edp/periodical/aa/2011/volume_532/issue_2011/aa16117-10/authorship/5
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The Herschel M 33 extended survey (HerM33es): PACS spectroscopy of the star-forming region BCLMP 302
Cool and warm dust emission from M 33 (HerM33es)
Variation in the dust emissivity index across M 33 with Herschel and Spitzer (HerM 33es)
Spectral energy distributions of H ii regions in M 33 ( HerM33es)
Cool gas and dust in M 33: Results from the HERschel M 33 Extended Survey (HERM33ES)
The AMIGA sample of isolated galaxies
The AMIGA sample of isolated galaxies
The Herschel M 33 extended survey (HerM33es): PACS spectroscopy of the star forming region BCLMP 302 (Corrigendum)
Dust and gas power spectrum in M 33 (HERM33ES)
Measuring star formation with resolved observations: the test case of M 33
Catalogues of isolated galaxies, isolated pairs, and isolated triplets in the local Universe
Star Formation in M 33 (HerM33es)
The AMIGA sample of isolated galaxies
Star formation and gas in the minor merger UGC 10214
On the nature of faint mid-infrared sources in M 33
H I asymmetry in the isolated galaxy CIG 85 (UGC 1547)
Gas and dust cooling along the major axis of M 33 ( HerM33es)
Dust properties in H II regions in M 33
The AMIGA sample of isolated galaxies ( Corrigendum)
Star formation in M 33: the radial and local relations with the gas
Properties of compact 250 μm emission and H II regions in M 33 (HERM33ES)
PACS and SPIRE photometer maps of M 33: First results of the HERschel M 33 Extended Survey (HERM33ES)
Dense gas in M 33 ( HerM33es)
Effects of the environment on galaxies in the Catalogue of Isolated Galaxies: physical satellites and large scale structure
Millimeter and submillimeter excess emission in M 33 revealed by Planck and LABOCA
The effect of local and large-scale environments on nuclear activity and star formation
Radio synchrotron spectra of star-forming galaxies
Spatially resolving the dust properties and submillimetre excess in M 33
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