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The mass-metallicity relation of zCOSMOS galaxies at z ~ 0.7, its dependence on SFR, and the existence of massive low-metallicity galaxies, , , , , , , and . (2014)cite arxiv:1410.7389Comment: Submitted to A&A; 11 pages, 6 figures.A superluminous supernova in high surface density molecular gas within the bar of a metal-rich galaxy, , , , , , , , , and 1 other author(s). (2019)cite arxiv:1906.00972Comment: Accepted for publication in the Astrophysical Journal (ApJ).Cosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaitre-Tolman-Bondi model, , , , , , , , , and 2 other author(s). (2013)cite arxiv:1308.2199Comment: 23 pages, 11 figures. Accepted for publication in A&A.The evolution of the dust and gas content in galaxies, , , , , , , , , and 29 other author(s). (2013)cite arxiv:1311.3670Comment: Accepted for publication in A&A.On the redshift evolution (0 < z < 4) of dust attenuation and of the total (UV+IR) star formation rate density, , , , , , , , , and 12 other author(s). (2013)cite arxiv:1304.7000Comment: Submitted to A&A.An extremely young massive clump forming by gravitational collapse in a primordial galaxy, , , , , , , , , and 2 other author(s). (2015)cite arxiv:1505.01290Comment: Published in May 7 issue of Nature (http://dx.doi.org/10.1038/nature14409).The host galaxy of GRB 980425 / SN1998bw: a collisional ring galaxy, , , , , , , , , and 1 other author(s). (2019)cite arxiv:1903.00485Comment: Accepted for publication in MNRAS. For the definitive version visit 'https://academic.oup.com/mnras'.Evolution of the specific Star Formation Rate Function at z<1.4 - Dissecting the mass-SFR plane in COSMOS and GOODS, , , , , , , , , and 12 other author(s). (2014)cite arxiv:1410.4875Comment: 24 pages, 15 figures, 3 tables, submitted to A&A, comments are welcome.Mass and metallicity scaling relations of high redshift star-forming galaxies selected by GRBs, , , , , , , , , and 12 other author(s). (2017)cite arxiv:1709.06574Comment: Accepted for publication in MNRAS.A Molecular gas rich GRB host galaxy at the peak of cosmic star formation with significant outflowing gas, , , , , , , , , and 3 other author(s). (2017)cite arxiv:1709.00424Comment: Submitted to MNRAS Letters.