ALMA Large Program FAUST (Fifty AU STudy of the chemistry in the disk/envelope systems of Solar-like protostars)
FAUST
Progetto
Progetto
RSN2
Attività: Nuova; Data inizio: 2018; Data fine: 2028
claudio.codella claudio.codella@inaf.it
FAUST è un progetto basato sul primo Large Program ALMA focalizzato all'astrochimica di regioni di formazione stellare di tipo Solare. co-led by INAF (C. Codella). L'obiettivo principale e' lo studio delle proprieta' fisco-chimiche delle regioni protostellari su varie scale spaziali, dall'envelope (2000 au) ai dischi protoplanetari su scale del Sistema Solare (< 50 au). Che mix di gas (Complex Organics) e polveri aveva il nostro Sistema Solare quando si e' formato? FAUST ha permesso ad ALMA di trovare/risolvere problemi legati alla calibrazione (https://help.almascience.org/kb/articles/what-errors-could-originate-from-the-correlator-spectral-normalization-and-tsys-calibration). Come conseguenza, la consegna dei dati finali sarà completata entro la fine di Aprile 2024.
FAUST is the first ALMA LP (co-led by INAF) on astrochemistry. The huge variety of planetary systems discovered depends on the early history of their formation. The goal is to reveal/quantify the chemical composition of the envelope/disk system in a sample of Class 0/I protostars, namely (1) to disentangle the components of the 50-2000 au envelope/disk system, (2) to characterise the organic, (3) to probe their ionization structure, and (4) to measure deuteration (http://faust-alma.riken.jp). Final datacubes calibration was challenging: FAUST allowed ALMA to fix calibration issues (https://help.almascience.org/kb/articles/what-errors-could-originate-from-the-correlator-spectral-normalization-and-tsys-calibration). Thus, the final dataset will be completed by the end of 2024 April.
Mezzo interstellare, formazione di stelle e sistemi planetari
Origine ed evoluzione dei pianeti, satelliti e corpi minori
Bioastronomia, Astrobiologia e Astrofisica di laboratorio
Infrastrutture da Terra (utilizzo)
Comunicazione, Didattica, Divulgazione
| Struttura | Nfte | N0 | TI 2024 | TI 2025 | TI 2026 | TD 2024 | TD 2025 | TD 2026 | Nex | Extra |
|---|---|---|---|---|---|---|---|---|---|---|
| O.A. ARCETRI | 4 | 0 | 0.40 | 0.40 | 0.40 | 0.50 | 0.50 | 0.50 | 0 | 0.00 |
| Totali | 4 | 0 | 0.40 | 0.40 | 0.40 | 0.50 | 0.50 | 0.50 | 0 | 0.00 |
| # | Struttura | TI 2024 | TI 2025 | TI 2026 | TD 2024 | TD 2025 | TD 2026 | Extra |
|---|---|---|---|---|---|---|---|---|
| 1 | ESO Research Fellow - Garching | 0 | 0 | 0 | 0.30 | 0.30 | 0.30 | 0.00 |
| 2 | ORIGINS - Vera Rubin Research Fellow | 0 | 0 | 0 | 0.30 | 0.30 | 0.30 | 0.00 |
| Totali | 0.00 | 0.00 | 0.00 | 0.60 | 0.60 | 0.60 | 0.00 |
| Certi 2024 | Certi 2025 | Certi 2026 | Presunti 2024 | Presunti 2025 | Presunti 2026 |
|---|---|---|---|---|---|
| 91.0 | 0.0 | 0.0 | 0.0 | 0.0 | 0.0 |
Astrochemistry - Astrobiology - Planetary disks - Protostars - Young Stellar Objects - Interstellar Medium - Interstellar Emission - Interstellar Molecules. The FAUST project is part of the ASTROCHEMISTRY@INAF - PROTOPLANETARY program.
C. Codella (INAF OAA) is co-PI of the project. In addition, INAF OAA is also coordinating (in synergy with RIKEN, Tokyo) the Work Package on the selection of Sources, verifying that the continuum and line datasets are fully exploited.
ALMA; VLA: SKA-MeerKAT+
| # | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2024/2025/2026) | FTE Presunte (2024/2025/2026) | Extra | ||
|---|---|---|---|---|---|---|---|---|---|---|
| 1 | claudio.codella | claudio.codella@inaf.it | O.A. ARCETRI | Y | DIRIGENTE DI RICERCA | Primo Ricercatore - co-PI di FAUST - Chemical complexity in protostellar and protoplanetary disks | X X X | X X X | X |
|
| 2 | francesco.fontani | francesco.fontani@inaf.it | O.A. ARCETRI | Y | PRIMO RICERCATORE | Ricercatore - Molecular Fractionation and Deuteration | X X X | X X X | X |
|
| 3 | linda.podio | linda.podio@inaf.it | O.A. ARCETRI | Y | PRIMO RICERCATORE | Ricercatore; chemical complexity in protostellar and protoplanetary disks | X X X | X X X | X |
|
| 4 | davide.fedele | davide.fedele@inaf.it | O.A. ARCETRI | Y | PRIMO RICERCATORE | Ricercatore - Analysis of dust continuum emission | X X X | X X X | X |
|
| 5 | giovanni.sabatini | giovanni.sabatini@inaf.it | O.A. ARCETRI | N | RICERCATORE | Chemical evolution of protostellar regions - comparison with high-mass SFRs | X X X | X X X | X |
|
| # | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2024/2025/2026) | FTE Presunte (2024/2025/2026) | Extra | |
|---|---|---|---|---|---|---|---|---|---|
| 1 | marta.desimone | marta.desimone@eso.org | ESO Research Fellow - Garching | N | ESO Fellow, INAF associated | Molecular complexity of the earliest (protostellar) evolutionary stages of Sun-like analogs - Observations and Modelling | [0.3, 0.3, 0.3] | [-1.0, -1.0, -1.0] | -1.0 |
| 2 | eleonora.bianchi | eleonora.bianchi@origins-cluster.de | ORIGINS - Vera Rubin Research Fellow | N | Vera Rubin Fellow, INAF associated | Interstellar organics and large carbon chains from protoplanetary objects to comets - Observations and modelling | [0.3, 0.3, 0.3] | [-1.0, -1.0, -1.0] | -1.0 |
The context of this project was awarded by INAF, EU fundings: (1) ASTRO-CHEMICAL ORIGINS (ACO) ITN H2020 EC MARIE SKŁODOWSKA-CURIE ACTIONS, PI C. Ceccarelli (Total: 4138 kEuro; Total INAF: 392 KEuro), (2) the INAF-GO 2023 fundings PROTO-SKA (Exploiting ALMA data to study planet forming disks: preparing the advent of SKA, PI: C. Codella, Total: 50 kEuro)
| # | Provenienza | Certi 2024 (k€) | Certi 2025 (k€) | Certi 2026 (k€) | Presun. 2024 (k€) | Presun. 2025 (k€) | Presun. 2026 (k€) | Totale Certi (k€) | Totale Presunti (k€) |
|---|---|---|---|---|---|---|---|---|---|
| 1 | H2020 ITN EU ACO | 41 | 0 | 0 | 0 | 0 | 0 | 41 | 0 |
| 2 | PROTO-SKA | 50 | 0 | 0 | 0 | 0 | 0 | 50 | 0 |
| # | Provenienza | Fondi 2024 (€) | Fondi 2025 (€) | Fondi 2026 (€) |
|---|