Scheda FAUST
FINAL
Informazioni generali
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. PIship: INAF (C. Codella)-Uni Tokyo-RIKEN Tokyo-UGA France-NRAO USA. Il progetto gode anche di progetti osservativi complementari nel centimtrico (VLA). 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 Organic species) e polveri aveva il nostro Sistema Solare quando si e' formato? La consegna dei dati finali (13 sorgenti, ognuna osservata con due 12 m arrays + ACA), è iniziata nel Dicembre 2021 e sarà completata entro la fine di Aprile 2022.
FAUST is the first ALMA LP (co-led by INAF) on astrochemistry. The huge variety of planetary systems discovered in recent decades likely depends on the early history of their formation. The goal is to reveal and quantify the variety of chemical composition of the envelope/disk system in a sample of Class 0 and I protostars representative of the chemical diversity observed at larger scales, namely (1) to disentangle the components of the 50-2000 au envelope/disk system, (2) to characterize the organic, (3) to probe their ionization structure, and (4) to measure deuteration (http://faust-alma.riken.jp). The release of the final FAUST dataset (13 sources, each imaged using two 12-m arrays, 1 ACA track) is on-going: it started on 2021, December, and will be completed by the end of 2022 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
Team Summary
15. Personale INAF coinvolto
Numero di partecipanti INAF al progetto: 6
| Struttura | Nfte | N0 | TI 2022 | TI 2023 | TI 2024 | TD 2022 | TD 2023 | TD 2024 | Nex | Extra |
|---|---|---|---|---|---|---|---|---|---|---|
| O.A. ARCETRI | 4 | 0 | 0.60 | 0.40 | 0.40 | 0.00 | 0.00 | 0.00 | 2 | 0.30 |
| Totali | 4 | 0 | 0.60 | 0.40 | 0.40 | 0.00 | 0.00 | 0.00 | 2 | 0.30 |
16. Personale Associato INAF coinvolto
Numero di partecipanti Associati INAF: 2
| # | Struttura | TI 2022 | TI 2023 | TI 2024 | TD 2022 | TD 2023 | TD 2024 | Extra |
|---|---|---|---|---|---|---|---|---|
| 1 | IPAG - Grenoble | 0 | 0 | 0 | 0.60 | 0.60 | 0.60 | 0.00 |
| Totali | 0.00 | 0.00 | 0.00 | 0.60 | 0.60 | 0.60 | 0.00 |
Fondi a sostegno
21. Totale fondi a disposizione (dato aggregato, k€)
| Certi 2022 | Certi 2023 | Certi 2024 | Presunti 2022 | Presunti 2023 | Presunti 2024 |
|---|---|---|---|---|---|
| 38.0 | 38.0 | 0.0 | 0.0 | 0.0 | 0.0 |
Produzione scientifica e tecnologica
22. Produzione scientifica e tecnologica - Highlights
Informazioni Pubbliche
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+
15. Team members, Informazioni generali
15. Personale INAF coinvolto
| # | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2022/2023/2024) | FTE Presunte (2022/2023/2024) | Extra | ||
|---|---|---|---|---|---|---|---|---|---|---|
| 1 | claudio.codella | claudio.codella@inaf.it | O.A. ARCETRI | Y | PRIMO RICERCATORE | 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 | RICERCATORE | Ricercatore - Molecular Fractionation and Deuteration | X X X | X X X | X |
|
| 3 | linda.podio | linda.podio@inaf.it | O.A. ARCETRI | Y | 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 | RICERCATORE | Ricercatore - Analysis of dust continuum emission | X X X | X X X | X |
|
| 5 | seyma.mercimek | seyma.mercimek@inaf.it | O.A. ARCETRI | N | ASSEGNISTA | PhD student - IRAM and ALMA Analysis - Astrochemical modelling | X X X | X X X | X |
|
| 6 | lucy.evans | lucy.evans@inaf.it | O.A. ARCETRI | N | ASSOCIATO - DOTTORANDO STRUTTURE | PhD student - Chemical complexity of low-mass star forming regions | X X X | X X X | X |
|
16. Personale Associato INAF coinvolto
| # | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2022/2023/2024) | FTE Presunte (2022/2023/2024) | Extra | |
|---|---|---|---|---|---|---|---|---|---|
| 1 | marta.desimone | marta.desimone@univ-grenoble-alpes.fr | IPAG - Grenoble | N | postdoc, INAF associate | 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@univ-grenoble-alpes.fr | IPAG - Grenoble | N | postdoc, INAF associate | 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 |
21. Fondi a Sostegno Iniziativa
The context of this project (Astrochemistry of Sun-like star forming regions) was awarded by several MIUR, INAF, EU fundings: (1) PRIN-MIUR 2016 STAR IN THE CAOS PRIN-MIUR project (Simulation Tools for Astrochemical Reactivity and Spectroscopy in the Cyberinfrastructure for Astrochemical Organic Species) PI. V. Barone (Total: 180 kE; Total INAF 20 kEuro); (2) GENESIS-SKA PRIN-INAF project (GEneral conNditions in Early Planetary Systems for the rISe of life with SKA), PI C. Codella (Total: 408 kEuro); (3) ASTRO-CHEMICAL ORIGINS (ACO) ITN H2020 EC MARIE SKŁODOWSKA-CURIE ACTIONS, PI C. Ceccarelli (Total: 4138 kEuro; Total INAF: 392 KEuro). EU ACO have been focused to train PhD students, who are going to conclude their PhD projects at the end of 2022. Note, however, that the first two programs are over, while the ACO EU project is focused on the training of PhD students (who will conclude their projects this year), and it does not allow the recruitment of post-doctoral positions. As also reported in the comments provided by INAF on Scheda FAUST 2021, the INAF role would definitely benefit if post-docs with an expertise on astrochemistry could be assigned to this project. The final dataset started to be released on 2021 December and will be completed by the end of 2022 April. An experienced postdoc is needed to boost the publications led by INAF before data will be public.
Tabella fondi:
| # | Provenienza | Certi 2022 (k€) | Certi 2023 (k€) | Certi 2024 (k€) | Presun. 2022 (k€) | Presun. 2023 (k€) | Presun. 2024 (k€) | Totale Certi (k€) | Totale Presunti (k€) |
|---|---|---|---|---|---|---|---|---|---|
| 1 | H2020 ITN EU ACO | 38 | 38 | 0 | 0 | 0 | 0 | 76 | 0 |
Tabella fondi Astrofisica Fondamentale e PNRR:
| # | Provenienza | Fondi 2022 (€) | Fondi 2023 (€) | Fondi 2024 (€) |
|---|