Team
A brief description of the team composition and expertise is given below:
Osservatorio di Roma:
Brunella Nisini: PI of the YODA project. Expert in winds and outflows from YSOs at different wavelengths.
Simone Antoniucci: analysis of optical/IR data, AO imaging of jets. PI of the GHOsT program.
Katia Biazzo: stellar parameters, mass accretion at low metallicity. Co-I of JWST GTO of young clusters
Teresa Giannini: spectroscopic diagnostics of wind/jets, accretion variability in YSOs
Manuele Gangi: Analysis of optical/IR data, diagnostics of winds and accretion
Osservatorio di Arcetri:
Francesca Bacciotti: Optical/ALMA observations of jets and cavities, MHD models of jets
Claudio Codella: Analysis of sub-millimeter ALMA observations, diagnostics of winds and cavities in young Class 0/I sources
Linda Podio: Analysis of sub-millimeter ALMA observations, PI of the ALMA-DOT program
Antonio Garufi: Infrared/sub-mm high resolution imaging of disks and streamers
Davide Fedele: Analysis of sub-millimeter ALMA observations of gas and dust in disks, application of thermo-chemical models
Osservatorio di Capodimonte:
Juan AlcalĂ : Analysis of UV/optical observations from ULLYSES/PENELLOPE LP
Elvira Covino: Analysis of optical spectra, Stellar parameters
Alessio Caratti o Garatti; Analysis of infrared spectra, accretion in class0/I sources, co-I of JWST-MIRI GTO
Eleonora Fiorellino: Accretion in class I sources
Osservatorio di Catania:
Antonio Frasca: Analysis of optical/IR spectra, Tools for stellar parameters
Osservatorio di Padova:
Elisabetta Rigliaco: Coordinator of OAPd RU. Infrared high resolution imaging of streamers and outflow cavities, co-I of the SPHERE-DESTINYS LP
Raffaele Gratton: Optical/IR high SPHERE observations
Osservatorio di Palermo:
Rosaria Bonito: Analisi of optical spectra, mass accretion and variability
Mario Guarcello: Analisi of optical spectra, mass accretion in young clusters
Universita' di Milano:
Giuseppe Lodato: Models of MHD winds, Population synthesis tools under viscous and wind-driven accretion (DiskPop), co-I of the ExoALMA LP
Giovanni Rosotti (Leicester): Analytical thermo-chemical models for MHD disk winds, co-I of the AgePRO and ExoALMA ALMA LP
INAF Associates and external collaborators:
Claudia Toci (ESO) Radiative transfer codes for gas and dust disk distribution
Carlo Manara (ESO): PI PENELLOPE LP, Accretion diagnostics, ALMA observations of disks
Anna Miotello (ESO): ALMA observations of streamers and disks
Rebeca Garcia Lopez (DIAS): high resolution IR observations with GRAVITY@VLT
Barbara Ercolano (Munich University): Analytical thermo-chemical models for photo-evaporative disk winds