Scientific Highlights
Publications as first author :
- Magnelli, B., et al., “The far-infrared/radio correlation and radio spectral index of galaxies in the SFR-M∗ plane up to z ∼ 2”, 2015, A&A, 573, 45
PDF or ADS - Magnelli, B., et al., “The evolution of the dust temperatures of galaxies in the SFR-M∗ plane up to z ∼ 2”, 2014, A&A, 561, 86
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- Magnelli, B., et al., “The deepest Herschel-PACS far-infrared survey: number counts and infrared luminosity functions from combined PEP/GOODS-H observations”, 2013, A&A, 553, 132
PDF or ADS - Magnelli, B.., et al., “Dust temperature and CO→H2 conversion factor variations in the SFR-M∗ plane”, 2012, A&A, 548, 22
PDF or ADS - Magnelli, B., et al., “A Herschel view of the far-infrared properties of submillimetre galaxies”, 2012, A&A, 539, 155
PDF or ADS - Magnelli, B. et al., “Evolution of the dusty infrared luminosity function from z = 0 to z = 2.3 using observations from Spitzer”, 2011, A&A, 528, 35
PDF or ADS - Magnelli, B., et al., ”Far-infrared properties of submillimeter and optically faint radio galaxies”, 2010, A&A, 518, 28
PDF or ADS - Magnelli, B., Elbaz, D., Chary, R.R, Dickinson, M., Le Borgne, D., Frayer, D.T. & Willmer, C. N. A., “The 0.4 < z < 1.3 star formation history of the Universe as viewed in the far-infrared”, 2009, A&A, 496, 57
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- Magnelli, B., Chary, R.R, Pope, A., Elbaz, D., Morrison, G. & Dickinson, M., “IRAC Excess in Distant Star- Forming Galaxies: Tentative Evidence for the 3.3 μm Polycyclic Aromatic Hydrocarbon Feature?”, 2008, ApJ, 681, 258
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