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Prof. Roberto Maiolino
Qualifications 1992: MS in Physics, University of Florence 1996: PhD in Astronomy, University of Florence Main Academic Career 1992 -
1993: Fellowship at the Institute for Solid State Electronics (Roma, Italy) 1994 -
1995: Scholar at the Steward Observatory -
University of Arizona (Tucson, USA) 1995 -
1997: Postdoc at the Max-
Planck Institut fЭr Extraterrestrische Physik (Garching, Germany) 1997 -
2003: Staff Astronomer at the Arcetri Astrophysical Observatory (Firenze, Italy) 2003 -
2006: Associate Astronomer at the Arcetri Astrophysical Observatory 2006 -
2012: Associate Astronomer at the Astronomical Observatory of Rome 2012 -
present: Professor at the Cavendish Laboratory and at the Kavli Institute for Cosmology, University of Cambridge (UK), Chair of Experimental Astrophysics Other Appointments 2003 -
2005: ESO Observing Programmes Committee 2003 -
2006: IRAM Program Committee 2004: Chandra Time Allocation Committee 2005 -
2010: LBT Science and Technical Committee 2007 -
2008: ASTRONET Roadmap Working Group 2007 -
2011: European Science Advisory Committee (ESAC) for ALMA 2009 -
2011: LBT-
TNG Time Allocation Committee. 2009 -
2011: ASTRONET Wide Field Spectroscopy Working Group 2011 -
2012: EAS working group on the Future of European Space Astronomy 2013 -
2016: HIRES Steering Committee 2013 -
2016: SDSSIV-
Manga Strategic Composition Committee 2014: ESO committee for the planning of VLT in 2020's 2014 -
present: Scientific Council, Italian Embassy in London 2015 -
present: IAU Commission Organizing Committee X1 (Supermassive Black Holes, Feedback and Galaxy Evolution) 2016 -
present: JAXA's SPICA International Science Advisory Board 2016 -
present: Chair of the HIRES Science Advisory Team Major projects with leading roles or heavy involvement 2004 -
present: JWST -
NIRSpec Instrument Science Team 2005 -
present: Project Scientist of GIANO (TNG high resolution near-
IR spectrograph) 2008 -
2009: PI of the ESO Large Programme "AMAZE" 2008 -
2013: Project Scientist of SIMPLE (E-
ELT high resolution near-
IR spectrograph) 2011 -
present: Project Scientist of MOONS (next generation ESO-
VLT multi-
object near-
IR spectrograph) 2013 -
2016: UK Co-
PI of HIRES (E-
ELT High Resolution Spectrometer) 2016 -
present: Project Scientist of HIRES 2016-
present: Co-
PI of the ESO Large Programme KLEVER

Curriculum Vitae


Publications 302 refereed papers (and about 150 non-
refereed publications), cited more than 18,000 times, 50 papers cited more than 100 times, Hersh (h) factor of 73. Research and highlights I have been active in multiple areas of observational extragalactic astrophysics. The following are some of the main research areas, along with some of the associated highlights:


·

Galaxy formation in the early universe ь First detection of far-
infrared fine structure lines in galaxies at high redshift
(Maiolino et al. 2005, A&A 440, L51)
ь

Discovery of cold gas accreting onto a primeval galaxy at z>7 (Maiolino et al.
2015, MNRAS 452, 54)





·

Galactic outflows ь Discovery massive quasar-
driven molecular outflows (Feruglio, Maiolino et al.
2010, A&A 518, L155)
ь ь ь

Systemic characterization of massive quasar-
driven molecular outflows
(Cicone, Maiolino et al. 2014, A&A 562, A21)

First detection of massive quasar-
driven outflows at high redshift (Maiolino et al. 2010, MNRAS, 425, L66; Cicone, Maiolino et al. 2015, A&A 574, A14) First direct observational evidence of star formation quenching by quasar driven outflows (Cano-
Diaz, Maiolino et al. 2012, A&A 537, L8)

· Galaxy transformation and star formation quenching ь "Starvation" (or "strangulation", i.e. halt of gas inflow from the intergalactic medium) identified as primary mechanism responsible for terminating star formation in most galaxies (Peng, Maiolino & Cochrane et al. 2015, Nature 521,
192)

· Metallicity evolution throughout the cosmic epochs ь Determination of the evolution of the galaxy mass-
metallicity relation at z>3 and finding of a steep metallicity evolution of galaxies at z>3 (Maiolino et al.
2008, A&A 488, 463; Troncoso, Maiolino et al. 2014, A&A 563, A58)
ь

First measurements of metallicity gradients at z>3 and discovery of inverted gradients (Cresci, Mannucci, Maiolino et al. 2010, Nature 467, 811; Troncoso,
Maiolino et al. 2014, A&A 563, A58)

ь

Metallicity scaling relations with stellar mass, star formation rate, gas content, and environment (Mannucci, Cresci, Maiolino et al. 2010, MNRAS 408,
2115; Bothwell, Maiolino, et al. 2013, MNRAS 433, 1425; Bothwell, Maiolino et al. 2015, MNRAS 455, 1156; Peng & Maiolino 2014, MNRAS 438, 262; Nagao, Maiolino & Marconi 2006, A&A 459, 85) Metallicity determination of distant quasar host galaxies (Maiolino et al. 2003, ApJ 596, L155; Juarez et al. 2009, A&A 494, L25; Nagao, Marconi, Maiolino, 2006, A&A 447, 157; Nagao, Maiolino, Marconi, 2006, A&A 447, 863)

ь

· Formation and evolution of dust throughout the cosmic epochs ь Discovery of a supernova origin of dust at high redshift (Maiolino et al. 2004,
ь

Nature 431, 533, Stratta et al. 2007, ApJ 661, L9; Gallerani et al. 2010, A&A 523, A85) Cosmic evolution of the dust content in galaxies (Santini, Maiolino et al. 2014, A&A 562, A30)

· Unified model, circumnuclear medium and host galaxies of Active Galactic Nuclei


ь ь

Revision of the Unified Model through the introduction of a dual absorber
(Maiolino & Rieke 1995, ApJ 454, 95)

Discovery of a large population of heavily obscured AGNs (Maiolino et al. 1998,
A&A 488, 463; Risaliti, Maiolino & Salvati 1999, ApJ 522, 157; Bassani, Dadina, Maiolino et al. 1999, ApJS 121, 473) Dust absorption in AGNs and inconsistency with X-
ray gas absorption (Maiolino et al. 2001, A&A 365, 28)

ь ь ь ь

Discovery of "cometary"-
like gas clouds orbiting supermassive black holes
(Maiolino et al. 2010, A&A 517, A47)

Analysis of the dust covering factor in AGNs (Maiolino et al. 2007, A&A 468,
979)

Identification of a population of "Elusive AGNs" (Maiolino et al. 2003, MNRAS
344, L59; Risaliti, Maiolino et al. 2006, MNRAS 365, 303; Imanishi, Dudley, Maiolino et al. 2007, ApJS 171, 72) Star formation and stellar population in AGN host galaxies (Maiolino et al. 1995, Maiolino et al. 1998, Oliva, Origlia, Maiolino, Moorwood 1999, A&A 350, 9; Risaliti, Gilli, Maiolino, Salvati 2000, A&A 357, 13; Maiolino et al. 2005; Maiolino et al. 2007, A&A 468, 979; Santini et al. 2012, A&A 540, A109); Gas content in AGN host galaxies (Maiolino et al. 1997, ApJ 446, 561; Maiolino et al. 2007, A&A 472, L33; Vito, Maiolino et al. 2014, MNRAS 441, 1059) Evolution of the Black Hole-
Galaxy scaling relations (Lamastra, Menci, Maiolino et al. 2010, MNRAS, 405, 29; Bongiorno, Maiolino, et al. 2014, MNRAS 443, 2077; Marconi, Axon, Maiolino et al. 2008, ApJ 678, 693)

ь

ь ь

· · Warm-
Hot Intergalactic Medium ь Detection of diffuse soft X-
ray emission, associated with galaxy overdensities, tracing warm-
hot baryons in the intergalactic medium
(Zappacosta, Maiolino et al. 2005, MNRAS 357, 929; Zappacosta, Mannucci, Maiolino, et al. 2002, A&A 394, 7; Zappacosta, Maiolino et al. 2005, A&A 434, 801)

Obscured Supernovae ь Discovery of the first near-
infrared selected, obscured supernovae (Maiolino
et al. 2002, A&A 389, 84)

Teaching Lecturer at five international advanced schools since 2007. 2001-
2002, course "Extragalactic Astronomy and Cosmology", INAOE, Mexico 2007-
2008, course "Extragalactic Astrophysics", University of Rome III, Italy 2000-
2010, several lectures at the following universities: University of Florence (2005-
2006) University of Rome III (2005) University of Rome II, Tor Vergata (2008-
2009) International School for Advanced Studies, S.I.S.S.A (2008) 2012-
2013, postgraduate course "Astrophysical Techniques", Department of Physics, University of Cambridge 2013-
present, undergraduate Lab 1B Head of Class, University of Cambridge 2014-
present, undergraduate Part III course "Structure formation in the Universe", University of Cambridge 2015-
present, examiner of undergraduate Part II course "Astrophysical Fluid Dynamics", University of Cambridge Supervised or co-
supervised about 30 graduate and undergraduate students and about 25 postdocs. Most of them currently are faculty at major research institutes, or have fellowship or postdocs positions at major astronomical institutes.