| Dust formation and survival in supernova ejecta S Bianchi, R Schneider Monthly Notices of the Royal Astronomical Society 378 (3), 973-982, 2007 | 513 | 2007 |
| A supernova origin for dust in a high-redshift quasar R Maiolino, R Schneider, E Oliva, S Bianchi, A Ferrara, F Mannucci, ... Nature 431 (7008), 533-535, 2004 | 343 | 2004 |
| Stellar sources of dust in the high-redshift Universe R Valiante, R Schneider, S Bianchi, AC Andersen Monthly Notices of the Royal Astronomical Society 397 (3), 1661-1671, 2009 | 291 | 2009 |
| The dust scaling relations of the Herschel Reference Survey L Cortese, L Ciesla, A Boselli, S Bianchi, H Gomez, MWL Smith, ... Astronomy & Astrophysics 540, A52, 2012 | 230 | 2012 |
| The Herschel Reference Survey: dust in early-type galaxies and across the Hubble Sequence MWL Smith, HL Gomez, SA Eales, L Ciesla, A Boselli, L Cortese, ... The Astrophysical Journal 748 (2), 123, 2012 | 223 | 2012 |
| Dust spectral energy distributions of nearby galaxies: an insight from the Herschel Reference Survey L Ciesla, M Boquien, A Boselli, V Buat, L Cortese, GJ Bendo, S Heinis, ... Astronomy & Astrophysics 565, A128, 2014 | 205 | 2014 |
| The origin of the dust in high-redshift quasars: the case of SDSS J1148+ 5251 R Valiante, R Schneider, S Salvadori, S Bianchi Monthly Notices of the Royal Astronomical Society 416 (3), 1916-1935, 2011 | 202 | 2011 |
| The Herschel Virgo Cluster Survey-I. Luminosity function JI Davies, M Baes, GJ Bendo, S Bianchi, DJ Bomans, A Boselli, ... Astronomy & Astrophysics 518, L48, 2010 | 177 | 2010 |
| The extinction law at high redshift and its implications S Gallerani, R Maiolino, Y Juarez, T Nagao, A Marconi, S Bianchi, ... Astronomy & Astrophysics 523, A85, 2010 | 173 | 2010 |
| The first low-mass stars: critical metallicity or dust-to-gas ratio? R Schneider, K Omukai, S Bianchi, R Valiante Monthly Notices of the Royal Astronomical Society 419 (2), 1566-1575, 2012 | 165 | 2012 |
| Resolved 200 mu m images of nearby galaxies-evidence for an extended distribution of cold dust PB Alton, M Trewhella, R Evans, S Bianchi, W Gear, H Thronson, ... Astronomy & astrophysics 335 (3), 807-822, 1998 | 163 | 1998 |
| Monte Carlo simulations of dusty spiral galaxies: extinction and polarization properties S Bianchi, A Ferrara, C Giovanardi arXiv preprint astro-ph/9512083, 1995 | 162 | 1995 |
| The Herschel Virgo Cluster Survey-II. Truncated dust disks in H I-deficient spirals L Cortese, JI Davies, M Pohlen, M Baes, GJ Bendo, S Bianchi, A Boselli, ... Astronomy & Astrophysics 518, L49, 2010 | 157 | 2010 |
| Dust extinction and emission in a clumpy galactic disk-An application of the radiative transfer code TRADING S Bianchi Astronomy & Astrophysics 490 (1), 461-475, 2008 | 156 | 2008 |
| An atlas of Monte Carlo models of dust extinction in galaxies for cosmological applications A Ferrara, S Bianchi, A Cimatti, C Giovanardi The Astrophysical Journal Supplement Series 123 (2), 437, 1999 | 144 | 1999 |
| Vindicating single-T modified blackbody fits to Herschel SEDs S Bianchi Astronomy & Astrophysics 552, A89, 2013 | 143 | 2013 |
| Deep submillimeter images of NGC 891—Cold dust at larger Galactic radii PB Alton, S Bianchi, RJ Rand, EM Xilouris, JI Davies, M Trewhella The Astrophysical Journal 507 (2), L125, 1998 | 141 | 1998 |
| DustPedia: a definitive study of cosmic dust in the local universe JI Davies, M Baes, S Bianchi, A Jones, S Madden, M Xilouris, M Bocchio, ... Publications of the Astronomical Society of the Pacific 129 (974), 044102, 2017 | 139 | 2017 |
| Submillimetre photometry of 323 nearby galaxies from the Herschel Reference Survey L Ciesla, A Boselli, MWL Smith, GJ Bendo, L Cortese, S Eales, S Bianchi, ... Astronomy & Astrophysics 543, A161, 2012 | 138 | 2012 |
| Can Dust Emission Be Used to Estimate the Mass of the Interstellar Medium in Galaxies—A Pilot Project with the Herschel Reference Survey S Eales, MWL Smith, R Auld, M Baes, GJ Bendo, S Bianchi, A Boselli, ... The Astrophysical Journal 761 (2), 168, 2012 | 131 | 2012 |
Maarten BaesUniversiteit GentE-mail confirmado em ugent.be
