WEAVE Project: Galactic Archaeology (WEAVE-1)
WEAVE-GA (WEAVE-1)
Progetto
Progetto
Infrastruttura Inaf
RSN2
Infrastrutture
Attività: In Itinere; Data inizio: 2014; Data fine: 2026
antonella.vallenari antonella.vallenari@inaf.it
La formazione della Via Lattea come paradigma delle galassie spirali e' una questione fondamentale nella astrofisica moderna. Molte sono ancora le domande aperte: diverse popolazioni stellari hanno davvero origini diverse? Quale e'la importanza relativa dei processi interni (formazione stellare in situ, evoluzione secolare del disco, ecc) ed esterni (accrescimento di galassie, di gas...) nel formare la Galassia? Le Survey spettroscopiche WEAVE Galactic Archaeology (ammassi, disco, alone, galassie nane) al WHT si propongono di rispondere a queste domande con 5 anni (+2) di osservazione e piu' di 7 milioni di spettri
Many questions remain open in understanding how the complex structure of the Milky Way was
assembled, with its stellar populations occupying a bulge, a thin and thick disc and a halo. Whether the
different stellar populations have truly different origins, what the relative importance is of internal
(in-situ star formation, secular evolution of the disc, etc.) and external (accretion of galaxies, gas
accretions, etc.) processes in forming and shaping the Galaxy are questions to which the WEAVE@WHT Spectroscopic Galactic Archaeology surveys (clusters, disk, halo, dwarf galaxies) tries to find answers observing more than 7 millions of stellar spectra in 5(+2) years
Popolazioni e ammassi stellari galattici ed extragalattici
Struttura ed evoluzione stellare, incluse le fasi finali
Infrastrutture da Terra (utilizzo)
Struttura | Nfte | N0 | TI 2023 | TI 2024 | TI 2025 | TD 2023 | TD 2024 | TD 2025 | Nex | Extra |
---|---|---|---|---|---|---|---|---|---|---|
O.A. PADOVA | 3 | 0 | 0.50 | 0.60 | 0.60 | 0.00 | 0.00 | 0.00 | 0 | 0.00 |
OAS BOLOGNA | 4 | 0 | 0.40 | 0.40 | 0.40 | 0.60 | 0.60 | 0.60 | 1 | 0.10 |
O.A. CATANIA | 2 | 0 | 0.10 | 0.20 | 0.20 | 0.80 | 0.80 | 0.80 | 0 | 0.00 |
O.A. ARCETRI | 3 | 0 | 0.40 | 0.40 | 0.50 | 0.80 | 0.80 | 0.80 | 1 | 0.10 |
O.A. TRIESTE | 0 | 0 | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 1 | 0.30 |
O.A. BRERA | 0 | 0 | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 0 | 0.00 |
O.A. TORINO | 1 | 0 | 0.10 | 0.10 | 0.10 | 0 | 0 | 0 | 0 | 0.00 |
O.A. PALERMO | 0 | 0 | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 1 | 0.10 |
O.A. ROMA | 1 | 0 | 0.00 | 0.00 | 0.00 | 0.10 | 0.10 | 0.10 | 0 | 0.00 |
Totali | 14 | 0 | 1.50 | 1.70 | 1.80 | 2.30 | 2.30 | 2.30 | 4 | 0.60 |
# | Struttura | TI 2023 | TI 2024 | TI 2025 | TD 2023 | TD 2024 | TD 2025 | Extra |
---|---|---|---|---|---|---|---|---|
1 | Università di Catania | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 0.00 |
2 | Università di Bologna | 0.10 | 0.00 | 0.00 | 0 | 0 | 0 | 0.00 |
3 | Universita` di Firenze; | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 0.00 |
4 | Universita' di Padova | 0 | 0 | 0 | 0.00 | 0.00 | 0.00 | 0.00 |
5 | INAF OAS Bologna | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 0.00 |
6 | Universita' di Bologna | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 0.00 |
7 | Uni Parthenope | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 0.00 |
8 | UNIFI | 0 | 0 | 0 | 0.00 | 0.00 | 0.00 | 0.00 |
Totali | 0.10 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 |
Certi 2023 | Certi 2024 | Certi 2025 | Presunti 2023 | Presunti 2024 | Presunti 2025 |
---|---|---|---|---|---|
0.0 | 0.0 | 0 | 90.0 | 90.0 | 0 |
WEAVE Galactic and extragalactic astronomy; Milky Way Physics; Galactic abundances; Milky Way formation; Galactic Archaelogy; Milky Way evolution; Stellar astronomy: Star clusters; Globular clusters; Open clusters
<p>The role of INAF in the Instrument Consortium is described in the form WEAVE-0. INAF researchers are actively involved in several sub-surveys, from the disk, the halo, to the globular/open clusters, and the dwarf galaxies. Antonella Vallenari is the Italian PI and member of the Executive Board. She is the PI of the WEAVE survey Open Clusters. Angela Bragaglia is the Co-PI of the Open cluster survey, and member of the Survey Working Group in charge of the preparation of the observations. Sara Lucatello is the leader of the Calibration Working Group. Ricardo Carrera is member of the Quality Control Group in charge of validate the survey results. A. Antonio Frasca is the leader of young star pipeline, serving not only the OC survey but also the WEAVE Galactic Plane Survey (SCIP)<br></p>
WHT: WEAVE spectrograph; TNG: WEAVE User Archive, to disseminate the results to the scientific community; Cambridge Astronomical Survey Unit (CASU) data processing and intermediate data storage; ING data center; Trieste Data Center
# | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2023/2024/2025) | FTE Presunte (2023/2024/2025) | Extra | ||
---|---|---|---|---|---|---|---|---|---|---|
1 | antonella.vallenari | antonella.vallenari@inaf.it | O.A. PADOVA | Y | PRIMO RICERCATORE | National PI/Survey PI | X X X | X X X | X | |
2 | angela.bragaglia | angela.bragaglia@inaf.it | OAS BOLOGNA | Y | PRIMO RICERCATORE | deputy Survey PI/survey builder/SWG | X X X | X X X | X | |
3 | antonio.frasca | antonio.frasca@inaf.it | O.A. CATANIA | Y | RICERCATORE ASTRONOMO | young stars/builder | X X X | X X X | X | |
4 | donatella.romano | donatella.romano@inaf.it | OAS BOLOGNA | Y | RICERCATORE | chemical evolution models | X X X | X X X | X | |
5 | elena.franciosini | elena.franciosini@inaf.it | O.A. ARCETRI | Y | RICERCATORE ASTRONOMO | Li pipeline | X X X | X X X | X | |
6 | elena.pancino | elena.pancino@inaf.it | O.A. ARCETRI | Y | RICERCATORE | stellar characterisation | X X X | X X X | X | |
7 | gabriele.cescutti | gabriele.cescutti@inaf.it | O.A. TRIESTE | Y | RICERCATORE | chemical evolution model | X X X | X X X | X | |
8 | gisella.clementini | gisella.clementini@inaf.it | OAS BOLOGNA | N | ASSOCIATO QUIESCENTE | dwarf galaxies | X X X | X X X | X | |
9 | laura.magrini | laura.magrini@inaf.it | O.A. ARCETRI | Y | RICERCATORE | n-capture pipeline | X X X | X X X | X | |
10 | lorenzo.spina | spina.astro@gmail.com | O.A. PADOVA | N | ASSOCIATO ADR UNIVERSITA / ENTI | young stars | X X X | X X X | X | |
11 | maria.tsantaki | maria.tsantaki@inaf.it | O.A. ARCETRI | N | ASSEGNISTA | stellar parameters | X X X | X X X | X | |
12 | michele.bellazzini | michele.bellazzini@inaf.it | OAS BOLOGNA | Y | PRIMO RICERCATORE | dwaf galaxies | X X X | X X X | X | |
13 | monica.rainer | monica.rainer@inaf.it | O.A. BRERA | Y | TECNOLOGO | stellar characterisation | X X X | X X X | X | |
14 | nicoletta.sanna | nicoletta.sanna@inaf.it | O.A. ARCETRI | Y | RICERCATORE | Li abundances | X X X | X X X | X | |
15 | alessandro.spagna | alessandro.spagna@inaf.it | O.A. TORINO | Y | RICERCATORE | disk structure | X X X | X X X | X | |
16 | ronald.drimmel | ronald.drimmel@inaf.it | O.A. TORINO | Y | PRIMO TECNOLOGO | disk structure | X X X | X X X | X | |
17 | rosanna.sordo | rosanna.sordo@inaf.it | O.A. PADOVA | Y | RICERCATORE | stellar evolution | X X X | X X X | X | |
18 | sara.lucatello | sara.lucatello@inaf.it | O.A. PADOVA | Y | RICERCATORE | Calibration leader/ builder | X X X | X X X | X | |
19 | valentina.dorazi | valentina.dorazi@inaf.it | O.A. PADOVA | Y | RICERCATORE | stellar characterisation,globulars | X X X | X X X | X | |
20 | jimenez.carrera | jimenez.carrera@inaf.it | OAS BOLOGNA | N | RICERCATORE | Calibration, QAG, Survey Builder | X X X | X X X | X | |
21 | javier.alonso | javier.alonso@inaf.it | O.A. CATANIA | N | ASSEGNISTA | young star pipeline | X X X | X X X | X | |
22 | mathieu.van | mathieu.van@inaf.it | O.A. ARCETRI | N | ASSEGNISTA | n-capture element pipeline | X X X | X X X | X | |
23 | maria.randich | sofia.randich@inaf.it | O.A. ARCETRI | Y | DIRIGENTE DI RICERCA | chemical abundances, open clusters, Li | X X X | X X X | X | |
24 | richard.smart | richard.smart@inaf.it | O.A. TORINO | Y | PRIMO TECNOLOGO | input catalogs | X X X | X X X | X | |
25 | loredana.prisinzano | loredana.prisinzano@inaf.it | O.A. PALERMO | Y | RICERCATORE | young clusters | X X X | X X X | X | |
26 | gloria.andreuzzi | gloria.andreuzzi@inaf.it | O.A. ROMA | Y | RICERCATORE | chemical abundances | X X X | X X X | X | |
27 | paola.refiorentin | re_fiorentin@oato.inaf.it | O.A. TORINO | Y | RICERCATORE | Galactic kinematics | X X X | X X X | X | |
28 | giuseppe.bono | bono@roma2.infn.it | O.A. ROMA | N | ASSOCIATO CON INCARICO DI RICERC | variable stars, stellar models | X X X | X X X | X | |
29 | vittorio.braga | vittorio.braga@inaf.it | O.A. ROMA | N | RICERCATORE | variable stars, stellar models | X X X | X X X | X | |
30 | emanuele.dalessandro | emanuele.dalessandro@inaf.it | OAS BOLOGNA | Y | RICERCATORE | young clusters | X X X | X X X | X |
# | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2023/2024/2025) | FTE Presunte (2023/2024/2025) | Extra | |
---|---|---|---|---|---|---|---|---|---|
1 | alessandro.lanzafame | alessandro.lanzafame@inaf.it | Università di Catania | Y | Professore Associato | young stars | [0, 0, 0] | [0.0, 0.0, 0.0] | 0.0 |
2 | alessio.mucciarelli | alessio.mucciarelli2@unibo.it | Università di Bologna | Y | Professore Associato | globulars, dwarf galaxies, stellar populations | [0.1, 0, 0] | [0.0, 0.1, 0.1] | 0.0 |
3 | stefania.salvadori | stefania.salvadori@unifi.it | Universita` di Firenze; | Y | Professore Associato | dwarf galaxies | [0, 0, 0] | [0.0, 0.1, 0.0] | 0.0 |
4 | giuliano.iorio | giuliano.iorio@unipd.it | Universita' di Padova | N | Assegnista | stellar system simulations | [0, 0, 0] | [0.0, 0.0, 0.0] | 0.0 |
5 | monica.tosi | monica.tosi@inaf.it | INAF OAS Bologna | Y | Astronomo Ordinario in Quiescenza | stellar populations | [0, 0, 0] | [0.0, 0.0, 0.0] | 0.0 |
6 | andrea.miglio | andrea.miglio@unibo.it | Universita' di Bologna | Y | Professore Ordinario | stellar evolution, asteroseismology | [0, 0, 0] | [0.0, 0.0, 0.0] | 0.0 |
7 | laura.inno | laura.inno@inaf.it | Uni Parthenope | Y | Ricercatrice | open clusters, disk chemical abundances | [0, 0, 0] | [0.0, 0.0, 0.0] | 0.0 |
8 | asa.skuladottir | asa.skuladottir@unifi.it | UNIFI | N | RTD | dwarf galaxies, n-capture elements | [0, 0, 0] | [0.1, 0.1, 0.1] | 0.0 |
The Total cost to INAF to 2020 refers to the cost of the WEAVE-GA Science Consortium for survey preparation activities, excluding the activities already included in WEAVE-0 (pipeline preparation and validation). The INAF total cost refers to support operations and scientific exploitation. Tabella fondi refers to the cost of the WEAVE-1 part of the project. It includes 2 TD FTEs/y and costs for missions, hardware. The total cost of the WEAVE-GA International collaboration is derived scaling from INAF costs weighted on the number of participants See WEAVE: Project Overview for details
# | Provenienza | Certi 2023 (k€) | Certi 2024 (k€) | Certi 2025 (k€) | Presun. 2023 (k€) | Presun. 2024 (k€) | Presun. 2025 (k€) | Totale Certi (k€) | Totale Presunti (k€) |
---|---|---|---|---|---|---|---|---|---|
1 | INAF | 0 | 0 | None | 90 | 90 | None | 0 | 180 |
# | Provenienza | Fondi 2023 (€) | Fondi 2024 (€) | Fondi 2025 (€) |
---|---|---|---|---|
1 | INAF - Mini Grant | 0.0 |