A brief description of the team composition and expertise is given below:
Osservatorio di Capodimonte:
Juan Alcalà: PI of the SKYWALKER project, coordinator of the OANa RU and of the WP1. Expert on accretion in YSOs. Analysis of the Mid-IR, NIR data, and UV/optical observations from ULLYSES - PENELLOPE ESO-LP and ODYSSEUS.
Vincenzo Andretta: Expert on stellar atmosphere modeling. Analysis of chromospheric diagnostics
Antonio Armeni:
Elvira Covino: Analysis of optical spectra, Stellar parameters
Alessio Caratti o Garatti: Coordinator of WP0. Analysis of infrared (NIR and MidIR) spectra, accretion in Class 0/I sources, Co-I of JWST-MIRI GTO, and PI of the ERIS-GTO.
Samuel Federman:
Osservatorio di Catania:
Antonio Frasca: Coordinator of the OACt RU and of WP3, CoPI of the PENELLOPE collaboration. Analysis of optical/NIR spectra and photometry.
Giovanni Catanzaro: Analysis of optical/NIR spectra. Acquisition of optical spectra and photometry (SLN).
Innocenza Busà: Modeling of chromospheric diagnostics. Acquisition of optical spectra and photometry (SLN).
Javier Alonso Santiago: Analysis of optical/NIR spectra. Stellar parameters. Acquisition of optical spectra and photometry at the Serra la Nave (SLN) observatory.
Giovanni Occhipinti: Acquisition of optical spectra and photometry (SLN).
Osservatorio di Roma:
Brunella Nisini: Coordinator of the OARm RU and of WP2. Expert in winds and outflows from YSOs at different wavelengths.
Teresa Giannini: spectroscopic diagnostics of wind/jets, accretion variability in YSOs. PI of GLOROUS project.
Simone Antoniucci: analysis of AO-assisted optical/IR spectro-images. PI of scheda GHOsT.
Katia Biazzo: stellar parameters, mass accretion at low metallicity. Co-I of JWST GTO of young clusters
Maria Gabriela Navarro: reduction and analysis of JWST data. analysis of H2 emission in outflows.
Osservatorio di Arcetri:
Francesca Bacciotti: Coordinator of the OAAr RU and of WP2. Wind diagnostics in NIR/MIR and sub-mm (JWST, ALMA), comparison with MHD models.
Thomas Nony: Analysis of data from ALMA and JWST, comparison with properties of high mass protostellar systems
Linda Podio: PI of the ALMA-DOT program. Analysis of sub-millimeter ALMA observations, effects of astrochemistry on disk evolution.
Osservatorio di Torino:
Claudio Zanni: Coordinator of the OATo RU. Expert on the modeling of magnetic fields in YSOs and characterization of accretion regimes.
INAF Associates and external collaborators:
Carlo Manara (ESO/INAF): PI of PENELLOPE ESO-LP, Member of ODYSSEUS council. Accretion diagnostics, ALMA observations of disks.
Rebeca Garcia Lopez (UCD/INAF): high resolution IR observations with GRAVITY@VLT
Beate Stelzer (University of Tubingen): Expert on stellar magnetic activity and YSOs in the late phase of their evolution
Catherine Espaillat (Boston University): CoPI of the ODYSSEUS collaboration
Kevin France (University of Colorado): Observations and modeling of HST-UV spectroscopy, ODYSSEUS council member
Anna Miotello (ESO/Garching): ALMA observations of disks