Funded research projects
The list of the FUNDED PROJECTS that are present in the SURplus database, used by the University of Milano, follows here below.
The list of the FUNDED PROJECTS that are present in the SURplus database, used by the University of Milano, follows here below.
∧ ∨ Type | ∧ ∨ Title | Principal Investigators | Status | ∧ ∨ Year |
---|---|---|---|---|
PRIN10-11 - PRIN bando 2010-11 |
EVOLUZIONE CHIMICA E DINAMICA DELLA NOSTRA GALASSIA E DELLE GALASSIE DEL GRUPPO LOCALE
|
|
Closed | 2010 |
PRIN10-11 - PRIN bando 2010-11 |
Meccanica Statistica dei Sistemi Disordinati e Complessi
|
|
Closed | 2010 |
ASI - AGENZIA SPAZIALE ITALIANA |
Kinetic Inductane Detector for Space (KIDS)
|
|
Closed | 2016 |
CAR_EXT - CARIPLO - EXTRABANDO E PROGETTI TERRITORIALI |
Luini in nuova Luce - Indagini scientifiche su una selezione di opere di Bernardino Luini per un approfondimento delle conoscenze e lo sviluppo di un’attività di valorizzazione integrata
|
|
Closed | 2017 |
CONTR_AMPU - Contratti di ricerca finanziata da amministrazioni pubbliche |
Programma LSPE: installazione e campagna osservativa dello strumento STRIP
|
|
Closed | 2018 |
H20MCITNIF - Horizon 2020_Marie Skłodowska-Curie actions-Innovative Training Network (ITN)/Individual Fellowships (IF) |
Biomechanics in health and disease: advanced physical tools for innovative early diagnosis (Phys2BioMed)
|
|
Closed | 2018 |
H20MC_RISE - Horizon 2020_Marie Skłodowska-Curie actions-International and inter-sectoral cooperation through the Research and Innovation Staff Exchanges (RISE) |
Dust and gas in planet forming discs (DUSTBUSTER)
|
|
Closed | 2019 |
PNRA - Programma Nazionale di Ricerca in Antartide (MIUR) |
Proprietà ottiche di polveri eoliche in Antartide
|
|
Closed | 2017 |
H20MCITNIF - Horizon 2020_Marie Skłodowska-Curie actions-Innovative Training Network (ITN)/Individual Fellowships (IF) |
Collective effects and optomechanics in ultra-cold matter
|
|
Closed | 2017 |
H20_RIA - Horizon 2020_Research & Innovation Action/Innovation Action |
Beyond Planck -- delivering state-of-the-art observations of the microwave sky from 30 to 70 GHz for the next decade
|
|
Closed | 2018 |