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P-MaNGA Galaxies: Emission Lines Properties - Gas Ionisation and Chemical Abundances from Prototype Observations, , , , , , , , , and 20 other author(s). (2014)cite arxiv:1410.7781Comment: 37 pages, 28 figures, resubmitted to MNRAS after addressing the referee report.Zooming on the internal structure of $z\simeq6$ galaxies, , , , , and . (2016)cite arxiv:1609.01719Comment: 20 pages, 11 figures, submitted to MNRAS.EELT-HIRES the high-resolution spectrograph for the E-ELT, , , , , , , , , and 63 other author(s). (2016)cite arxiv:1609.00497Comment: 12 pages, in Ground-based and Airborne Instrumentation for Astronomy VI, 2016, Proc. SPIE 9908, 23.Resolved CII emission in a lensed quasar at z=4.4, , , , , , , , , and 2 other author(s). (2012)cite arxiv:1205.4035Comment: 7 pages, 5 figures, accepted for publication in A&A.Massive Molecular Outflows and Evidence for AGN Feedback from CO Observations, , , , , , , , , and 5 other author(s). (2013)cite arxiv:1311.2595Comment: 26 pages, Accepted for publication in A&A, abstract abridged due to arXiv requirements.Prospects for AGN studies with ALMA. (2008)cite arxiv:0806.0695Comment: 42 pages, 21 figures, Lecture notes for the school ÄGN at the highest angular resolution: theory and observations" (Torun), eds. A. Marconi and A. Niedzielski, New Astronomy Reviews, corrected a few typos.Observational evidence of quasar feedback quenching star formation at high redshift, , , , , and . \aap, (January 2012)Metallicity evolution, metallicity gradients and gas fractions at z~3.4, , , , , , , , , and 2 other author(s). (2013)cite arxiv:1311.4576Comment: Resubmitted to A&A after incorporating referee comments.Building the cosmic infrared background brick by brick with Herschel/PEP, , , , , , , , , and 17 other author(s). (2011)cite arxiv:1106.3070Comment: Proposed for acceptance on A&A.The Mean Star-Forming Properties of QSO Host Galaxies, , , , , , , , , and 15 other author(s). (2013)cite arxiv:1310.1922Comment: 10 figures, 1 table; accepted for publication in Astronomy & Astrophysics.