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Curriculum Vitae Leonardo Testi
March 2, 2005

Phone, e-mail: +390552752285, ltesti@arcetri.astro.it Degrees: Ph.D. in Astronomy, awarded in February 1997, Universit` degli Studi di Firenze; a "Laurea in fisica", June 7th 1993, full quotation cum laude, Universit` degli Studi di Firenze. a Positions: Astronomo Asso ciato, Istituto Nazionale di Astrofisica, May 2003 present Ricercatore Astronomo, Osservatorio Astrofisico di Arcetri, July 1998 May 2003 Postdo ctoral Scholar, California Institute of Technology, May 1997 - February 1999 Positions held in working groups and science p olicy commettes: ALMA Science Advisory Commettee, Memb er (2003), Chairman (2005) VITRUV/VLTI Science Working Group, Memb er (2005) ALMA Europ ean Science Advisory Commettee, Memb er (2003) AMBER/VLTI Science Working Group, Memb er (2001) ESO Observing Programme Commettee, Panel C Memb er (20022004), Memb er-at-large (2004) Spitzer Space Telescop e Observing Programme Commettee, Panel 4, Memb er (2004) NASA Origins of Solar Sistem Review Panel, Observations Subpanel, Memb er (1999) OVRO millimeter array Time Allo cation Commettee, Memb er (19971999) Main research interests My main scientific activities are related to observational studies of the formation and early evolution of stars and stellar clusters, the formation of substellar ob jects and the prop erties and evolution of circumstellar disks. Primary ob jectives are: i) the identification of massive protostars and the study of the formation and early evolution of young stellar clusters; ii) the determination of the distribution of pre-stellar core masses in cluster regions, through mm continuum and molecular line interferometric mosaicing; iii) the study at infrared wavelengths of young brown dwarfs with the goal of constraining their formation mechanism; iv) the structure and physical prop erties of circumstellar disks prob ed at high angular resolution with near infrared adaptive optics and interferometric techniques; v) the study of dust emission prop erties in the infrared through the mm and cm wavebands with the goal of constraining its evolution in circumstellar disks leading to the formation of planetesimals. Selected Pap ers: - Testi L., Felli M., Persi P., & Roth M., 1998,"HII and hot dust emission around young massive stars in G 9.62+0.19", A&A, 329, 233 - Testi L. & Sargent A.I., 1998, "Star formation in clusters: a survey of compact mm-wave sources in the Serpens core", ApJ, 508, L91 - Testi L., Palla F., Natta A., 1999, "The onset of cluster formation around Herbig Ae/Be stars", A&A, 342, 515 - Natta A. & Testi L., 2001, "Exploring Brown Dwarf Disks", A&A, 376, L22 - Testi L., Natta A., Shepherd D.S., Wilner D.J., 2003, "Large grains in the disk of CQ Tau", A&A, 403, 323 The complete publication list is available at: http://www.arcetri.astro.it/lt/pro jects/ele lav.p df