Scheda AGN feedback FINAL

Informazioni generali

Black hole winds/outflows and the baryon life-cycle of galaxies

AGN feedback

Programma

Progetto

RSN1

Attività: In Itinere; Data inizio: 2014; Data fine: 2023

L'obiettivo di questo programma è verificare se feedback da buchi neri (BN) e' il responsabile per il regolamento della crescita delle galassie massicce.
Il programma sarà realizzato sfruttando due risorse principali: a) la grande quantità di dati dedicati raccolti sulla strumentazione di punta (MUSE, SINFONI e ALMA per mappare gas ionizzati e molecolari nelle galassie ospiti di AGN, XMM per sondare i venti nucleari); b) un team esperto e affiatato, che conta sia ricercatori orientati all'osservazione che modellisti. Alla fine del nostro progetto otterremo vincoli alla fisica del feedback da BN. Se questo feedback non fosse una soluzione praticabile, saremmo costretti a cercare un nuovo driver fisico per il regolamento della crescita delle galassie massicce.

The goal of this program is to assess or disprove black hole (BH) feedback as the physical driver for the quenching of massive galaxies.
The program will be achieved exploiting two main assets: a) the large amount of dedicated data collected on today's flagship intrumentation (MUSE, SINFONI and ALMA to map ionized and molecular gas in AGN host galaxies, XMM to probe AGN nuclear winds); b) an experienced and close-knit team, counting both observation-oriented and model-oriented researchers.
At the end of our project we would quantitatively assess BH feedback physics.
Should BH feedback not be a viable solution, we would be forced to look for a new physical driver for the quenching of massive galaxies, probably an even more important result.

Galassie, AGN e loro evoluzione

Fisica degli oggetti compatti galattici ed extragalattici

Team Summary

15. Personale INAF coinvolto

Numero di partecipanti INAF al progetto: 38

Struttura	Nfte	TI 2022	TI 2023	TI 2024	TD 2022	TD 2023	TD 2024	Nex	Extra
OAS BOLOGNA	4	0.40	0.40	0.00	0	0	0	0	0.00
O.A. TRIESTE	4	0.30	0.30	0.20	1.00	1.00	0.00	0	0.00
IAPS ROMA	1	0.10	0.10	0.00	0.00	0.00	0.00	0	0.00
NAN	0	0.00	0.00	0.00	0	0	0	0	0.00
O.A. PADOVA	1	0.00	0.00	0.00	0.10	0.00	0.00	1	0.10
O.A. ROMA	3	0.40	0.40	0.00	0	0	0	1	0.10
O.A. BRERA	0	0	0	0	0.00	0.00	0.00	0	0.00
IASF MILANO	1	0	0	0	1.00	0.50	0.00	0	0.00
IRA BOLOGNA	1	0.10	0.10	0.00	0.00	0.00	0.00	1	0.10
O.A. CAGLIARI	1	0	0	0	0.10	0.10	0.00	0	0.00
O.A. CAPODIMONTE	0	0.00	0.00	0.00	0	0	0	0	0.00
O.A. ARCETRI	2	0.20	0.20	0.00	0	0	0	0	0.00
Totali	18	1.50	1.50	0.20	2.20	1.60	0.00	3	0.30

16. Personale Associato INAF coinvolto

Numero di partecipanti Associati INAF: 22

#	Struttura	TI 2022	TI 2023	TI 2024	TD 2022	TD 2023	TD 2024	Extra
1	Università di Bologna	0.10	0.10	0.10	0.20	0.10	0.00	0.00
2	Scuola Normale Superiore	0.00	0.00	0.00	0	0	0	0.00
3	Università degli Studi di Roma - Tor Vergata	0.20	0.20	0.00	0	0	0	0.00
4	Università Roma 3	0.10	0.10	0.00	0	0	0	0.00
5	Universita' di Trieste	0	0	0	0.00	0.00	0.00	0.00
6	Scuola Normale Superiore di Pisa	0.20	0.20	0.00	0	0	0	0.00
7	Universita' di Firenze	0.00	0.00	0.00	0	0	0	0.00
8	ASI	0.20	0.20	0.00	0	0	0	0.00
9	Universita' Roma Tre	0.10	0.10	0.00	0	0	0	0.00
10	Università di Firenze	0	0	0	0.00	0.00	0.00	0.00
11	Università di Trieste	0	0	0	1.00	1.00	0.00	0.00
12	Pontificia Universidad Catolica (Cile)	0	0	0	0.20	0.20	0.00	0.00
13	CAB MAdrid	0	0	0	0.10	0.10	0.00	0.00
14	Universita' Roma3	0.10	0.10	0.00	0.60	0.50	0.00	0.00
15	Università di Cardiff	0	0	0	0.20	0.20	0.00	0.00
16	SISSA	0	0	0	0.50	0.50	0.00	0.00
	Totali	1.00	1.00	0.10	2.80	2.60	0.00	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
130.0	0.0	0	0.0	0.0	0

Produzione scientifica e tecnologica

22. Produzione scientifica e tecnologica - Highlights

#	DOI	Descrizione
1	10.1093/mnras/stz255	Titolo: The AGN fuelling/feedback cycle in nearby radio galaxies I. ALMA observations and early results Autori:Ilaria Ruffa and Isabella Prandoni and Robert A Laing and Rosita Paladino and Paola Parma and Hans .... Publisher:Oxford University Press (OUP) Rivista: Monthly Notices of the Royal Astronomical Society Anno pubblicazione:2019
2	10.3847/1538-4357/ab1a3a	Titolo: Outflows in the Disks of Active Galaxies Autori:N. Menci and F. Fiore and C. Feruglio and A. Lamastra and F. Shankar and E. Piconcelli and E. Giall .... Publisher:American Astronomical Society Rivista: The Astrophysical Journal Anno pubblicazione:2019
3	https://doi.org/10.1051/0004-6361/201937292	Titolo: The WISSH quasars project Autori:L. Zappacosta and E. Piconcelli and M. Giustini and G. Vietri and F. Duras and G. Miniutti and M. B .... Publisher:EDP Sciences Rivista: Astronomy \& Astrophysics Anno pubblicazione:2020
4	10.3847/1538-4357/ab67bd	Titolo: Multiphase Gas Flows in the Nearby Seyfert Galaxy ESO428\textendashG014. Paper I Autori:C. Feruglio and G. Fabbiano and M. Bischetti and M. Elvis and A. Travascio and F. Fiore Publisher:American Astronomical Society Rivista: The Astrophysical Journal Anno pubblicazione:2020
5	10.1051/0004-6361/201936197	Titolo: The WISSH quasars project Autori:A. Travascio and L. Zappacosta and S. Cantalupo and E. Piconcelli and F. Arrigoni Battaia and M. Gi .... Publisher:EDP Sciences Rivista: Astronomy \& Astrophysics Anno pubblicazione:2020
6	10.1093/mnras/stz2410	Titolo: Constraints on high-J CO emission lines in z $\sim$ 6 quasars Autori:S Carniani and S Gallerani and L Vallini and A Pallottini and M Tazzari and A Ferrara and R Maiolin .... Publisher:Oxford University Press (OUP) Rivista: Monthly Notices of the Royal Astronomical Society Anno pubblicazione:2019
7	10.1051/0004-6361/201834372	Titolo: The MAGNUM survey: different gas properties in the outflowing and disc components in nearby active galaxies with MUSE Autori:M. Mingozzi and G. Cresci and G. Venturi and A. Marconi and F. Mannucci and M. Perna and F. Belfior .... Publisher:EDP Sciences Rivista: Astronomy \& Astrophysics Anno pubblicazione:2019
8	10.1051/0004-6361/202039057	Titolo: The WISSH quasars project Autori:M. Bischetti and C. Feruglio and E. Piconcelli and F. Duras and M. P\'erez-Torres and R. Herrer .... Publisher:EDP Sciences Rivista: Astronomy \& Astrophysics Anno pubblicazione:2021 We study the impact of active galactic nuclei (AGN) ionised outflows on star formation in high-redshift AGN host galaxies, by combining near-infrared integral field spectroscopic (IFS) observations, mapping the Hα emission and [O III]λ5007 outflows, with matched-resolution observations of the rest-frame far-infrared (FIR) emission. We present high-resolution ALMA Band 7 observations of eight X-ray selected AGN (L2 − 10 keV = 1043.8 − 1045.2 erg s−1) at z ∼ 2 from the SUPER (SINFONI Survey for Unveiling the Physics and Effect of Radiative feedback) sample, targeting the observed-frame 870 μm (rest-frame ∼260 μm) continuum at ∼2 kpc (0.2″) spatial resolution. The targets were selected among the SUPER AGN with an [O III] detection in the IFS maps and with a detection in the FIR photometry. We detected six out of eight targets with signal-to-noise ratio S/N ≳ 10 in the ALMA maps, from which we measured continuum flux densities in the range 0.27 − 2.58 mJy and FIR half-light radii (Re) in the range 0.8 − 2.1 kpc. The other two targets were detected with S/N of 3.6 and 5.9, which are insufficient for spatially resolved analysis. The FIR Re of our sample are comparable to other AGN and star-forming galaxies at a similar redshift from the literature. However, combining our sample with the literature samples, we find that the mean FIR size in X-ray AGN (Re = 1.16 ± 0.11 kpc) is slightly smaller than in non-AGN (Re = 1.69 ± 0.13 kpc). From spectral energy distribution fitting, we find that the main contribution to the 260 μm flux density is dust heated by star formation, with ≤4% contribution from AGN-heated dust and ≤1% from synchrotron emission. The majority of our sample show different morphologies for the FIR (mostly due to reprocessed stellar emission) and the ionised gas emission (Hα and [O III], mostly due to AGN emission). This could be due to the different locations of dust and ionised gas, the different sources of the emission (stars and AGN), or the effect of dust obscuration. We are unable to identify any residual Hα emission, above that dominated by AGN, that could be attributed to star formation. Under the assumption that the FIR emission is a reliable tracer of obscured star formation, we find that the obscured star formation activity in these AGN host galaxies is not clearly affected by the ionised outflows. However, we cannot rule out that star formation suppression is happening on smaller spatial scales than the ones we probe with our observations (< 2 kpc) or on different timescales.
9	10.1051/0004-6361/202141363	Titolo: SUPER Autori:I. Lamperti and C. M. Harrison and V. Mainieri and D. Kakkad and M. Perna and C. Circosta and J. Sc .... Publisher:EDP Sciences Rivista: Astronomy \& Astrophysics Anno pubblicazione:2021 Abstract. We study the impact of active galactic nuclei (AGN) ionised outflows on star formation in high-redshift AGN host galaxies, by combining near-infrared integral field spectroscopic (IFS) observations, mapping the Hα emission and [O III]λ5007 outflows, with matched-resolution observations of the rest-frame far-infrared (FIR) emission. We present high-resolution ALMA Band 7 observations of eight X-ray selected AGN (L2 − 10 keV = 1043.8 − 1045.2 erg s−1) at z ∼ 2 from the SUPER (SINFONI Survey for Unveiling the Physics and Effect of Radiative feedback) sample, targeting the observed-frame 870 μm (rest-frame ∼260 μm) continuum at ∼2 kpc (0.2″) spatial resolution. The targets were selected among the SUPER AGN with an [O III] detection in the IFS maps and with a detection in the FIR photometry. We detected six out of eight targets with signal-to-noise ratio S/N ≳ 10 in the ALMA maps, from which we measured continuum flux densities in the range 0.27 − 2.58 mJy and FIR half-light radii (Re) in the range 0.8 − 2.1 kpc. The other two targets were detected with S/N of 3.6 and 5.9, which are insufficient for spatially resolved analysis. The FIR Re of our sample are comparable to other AGN and star-forming galaxies at a similar redshift from the literature. However, combining our sample with the literature samples, we find that the mean FIR size in X-ray AGN (Re = 1.16 ± 0.11 kpc) is slightly smaller than in non-AGN (Re = 1.69 ± 0.13 kpc). From spectral energy distribution fitting, we find that the main contribution to the 260 μm flux density is dust heated by star formation, with ≤4% contribution from AGN-heated dust and ≤1% from synchrotron emission. The majority of our sample show different morphologies for the FIR (mostly due to reprocessed stellar emission) and the ionised gas emission (Hα and [O III], mostly due to AGN emission). This could be due to the different locations of dust and ionised gas, the different sources of the emission (stars and AGN), or the effect of dust obscuration. We are unable to identify any residual Hα emission, above that dominated by AGN, that could be attributed to star formation. Under the assumption that the FIR emission is a reliable tracer of obscured star formation, we find that the obscured star formation activity in these AGN host galaxies is not clearly affected by the ionised outflows. However, we cannot rule out that star formation suppression is happening on smaller spatial scales than the ones we probe with our observations (< 2 kpc) or on different timescales.
10	10.1051/0004-6361/202039773	Titolo: The IBISCO survey Autori:M. V. Zanchettin and C. Feruglio and M. Bischetti and A. Malizia and M. Molina and A. Bongiorno and .... Publisher:EDP Sciences Rivista: Astronomy \& Astrophysics Anno pubblicazione:2021 Abstract: We present the analysis of the ALMA CO(2−1) emission line and the underlying 1.2 mm continuum of Mrk 509 with spatial resolution of ∼270 pc. This local Seyfert 1.5 galaxy, optically classified as a spheroid, is known to host an ionised disc, a starburst ring, and ionised gas winds on both nuclear (ultra-fast outflows) and galactic scales. From CO(2−1) we estimate a molecular gas reservoir of MH2 = 1.7 × 109 M⊙, located within a disc of size ∼5.2 kpc, with Mdyn = (2.0 ± 1.1) × 1010 M⊙ inclined at 44 ± 10 deg. The molecular gas fraction within the disc is μgas = 5%, consistent with that of local star-forming galaxies with similar stellar mass. The gas kinematics in the nuclear region within r ∼ 700 pc, that is only marginally resolved at the current angular resolution, suggests the presence of a warped nuclear disc. Both the presence of a molecular disc with ongoing star formation in a starburst ring, and the signatures of a minor merger, are in agreement with the scenario where galaxy mergers produce gas destabilisation, feeding both star formation and AGN activity. The spatially resolved Toomre Q-parameter across the molecular disc is in the range Qgas = 0.5 − 10, and shows that the disc is marginally unstable across the starburst ring, and stable against fragmentation at nucleus and in a lopsided ring-like structure located inside of the starburst ring. We find complex molecular gas kinematics and significant kinematics perturbations at two locations, one within 300 pc of the nucleus and one 1.4 kpc away close to the region with high Qgas, that we interpret as molecular winds with velocity v98 = 200 − 250 km s−1. The total molecular outflow rate is in the range 6.4−17.0 M⊙ yr−1 for the optically thin and thick cases, respectively. The molecular wind total kinetic energy is consistent with a multiphase momentum-conserving wind driven by the AGN with Ṗof/Ṗrad in the range 0.06−0.5. The spatial overlap of the inner molecular wind with the ionised wind, and their similar velocity suggest a cooling sequence within a multiphase wind driven by the AGN. The second outer molecular wind component overlaps with the starburst ring, and its energy is consistent with a supernova-driven wind arising from the starburst ring.

Informazioni Pubbliche

Active galactic nuclei; AGN host galaxies; Radio galaxies; Quasars; Radio jets; Seyfert galaxies; X-ray active galactic nuclei; Interstellar medium; Circumgalactic medium; GAEA; XQR-30; HYPERION

INAF is the leader of project PRIN MIUR BLACKOUT (PI Fabrizio Fiore). The Task leaders are all INAF personel or INAF Associates (https://blackholewinds.inaf.it/index.php/science/work-packages/). INAF personnel leads 4 Tasks, and participates in the other 7 Tasks. 4 Tasks led by INAF: T1.1 Luminous quasars at z=3-4; T3.2 IBISCO survey; T3.3 EIFFEL survey; T4.2 Semi-analytical models. <div> </div>

CTA, MAGIC, LBT; TNG; ESO (ALMA, VLT/Sinfoni, VLT/X-shooter, VLT/MUSE,VLT/VIMOS); ESA (XMM-Newton, Herschel), NASA (WISE, HST, Chandra);SDSS; JVLA; NOEMA.

15. Team members, Informazioni generali

15. Personale INAF coinvolto

#	Nome	E-mail	Struttura	TI	Qualifica	Ruolo nel Progetto	FTE Impegnate (2022/2023/2024)	FTE Presunte (2022/2023/2024)	Extra
1	eleonora.torresi	eleonora.torresi@inaf.it	OAS BOLOGNA	Y	RICERCATORE	data analisi	X X X	X X X	X
2	fabrizio.fiore	fabrizio.fiore@inaf.it	O.A. TRIESTE	Y	DIRIGENTE DI RICERCA	coordinamento	X X X	X X X	X
3	fabio.fontanot	fabio.fontanot@inaf.it	O.A. TRIESTE	Y	RICERCATORE	sviluppo modelli	X X X	X X X	X
4	francesca.panessa	francesca.panessa@inaf.it	IAPS ROMA	Y	RICERCATORE	data analisi	X X X	X X X	X
5	gabriele.bruni	gabriele.bruni@inaf.it	IAPS ROMA	N	RICERCATORE	data analisi	X X X	X X X	X
6	massimo.gaspari	massimo.gaspari@inaf.it	NAN	Y	RICERCATORE	sviluppo modelli	X X X	X X X	X
7	andrea.grazian	andrea.grazian@inaf.it	O.A. PADOVA	Y	RICERCATORE	data analisi	X X X	X X X	X
8	giorgio.lanzuisi	giorgio.lanzuisi@inaf.it	OAS BOLOGNA	Y	RICERCATORE	data analisi	X X X	X X X	X
9	angela.malizia	angela.malizia@inaf.it	OAS BOLOGNA	Y	RICERCATORE	data analisi	X X X	X X X	X
10	manuela.bischetti	manuela.bischetti@units.it	O.A. TRIESTE	N	ASSOCIATO	data analisi	X X X	X X X	X
11	massimo.cappi	massimo.cappi@inaf.it	OAS BOLOGNA	Y	PRIMO RICERCATORE	data analisi	X X X	X X X	X
12	mauro.dadina	mauro.dadina@inaf.it	OAS BOLOGNA	Y	RICERCATORE	data analisi	X X X	X X X	X
13	nicola.menci	nicola.menci@inaf.it	O.A. ROMA	Y	ASTRONOMO ASSOCIATO	sviluppo modelli	X X X	X X X	X
14	enrico.piconcelli	enrico.piconcelli@inaf.it	O.A. ROMA	Y	RICERCATORE	coordinamento e data analisi	X X X	X X X	X
15	emanuele.giallongo	emanuele.giallongo@inaf.it	O.A. ROMA	Y	ASTRONOMO ORDINARIO	data analisi	X X X	X X X	X
16	gabriele.ponti	gabriele.ponti@inaf.it	O.A. BRERA	N	PRIMO RICERCATORE	data analisi	X X X	X X X	X
17	andrea.travascio	andrea.travascio@inaf.it	O.A. TRIESTE	N	ASSOCIATO ADR UNIVERSITA / ENTI	data analisi	X X X	X X X	X
18	giustina.vietri	giustina.vietri@inaf.it	IASF MILANO	N	RICERCATORE	data analisi	X X X	X X X	X
19	luca.zappacosta	luca.zappacosta@inaf.it	O.A. ROMA	Y	RICERCATORE	data analisi	X X X	X X X	X
20	isabella.prandoni	prandoni@ira.inaf.it	IRA BOLOGNA	Y	PRIMO RICERCATORE	coordinamento	X X X	X X X	X
21	rosita.paladino	rosita.paladino@inaf.it	IRA BOLOGNA	Y	RICERCATORE	data analisi	X X X	X X X	X
22	viviana.casasola	viviana.casasola@inaf.it	IRA BOLOGNA	Y	RICERCATORE	data analisi	X X X	X X X	X
23	paola.parma	p.parma@ira.inaf.it	IRA BOLOGNA	N	ASSOCIATO QUIESCENTE	data analisi	X X X	X X X	X
24	filippo.maccagni	filippo.maccagni@inaf.it	O.A. CAGLIARI	N	ASSOCIATO	data analisi	X X X	X X X	X
25	marilena.spavone	marilena.spavone@inaf.it	O.A. CAPODIMONTE	Y	TECNOLOGO	data analisi	X X X	X X X	X
26	giulia.migliori	giulia.migliori@inaf.it	IRA BOLOGNA	Y	RICERCATORE	data analisi	X X X	X X X	X
27	susanna.bisogni	susanna.bisogni@inaf.it	IASF MILANO	N	RICERCATORE	data analisi	X X X	X X X	X
28	filippo.mannucci	filippo.mannucci@inaf.it	O.A. ARCETRI	Y	DIRIGENTE DI RICERCA	data analisi	X X X	X X X	X
29	giovanni.cresci	giovanni.cresci@inaf.it	O.A. ARCETRI	Y	RICERCATORE	coordinamento e data analisi	X X X	X X X	X
30	emanuele.nardini	emanuele.nardini@inaf.it	O.A. ARCETRI	Y	RICERCATORE	data analisi	X X X	X X X	X
31	antonino.marasco	antonino.marasco@inaf.it	O.A. PADOVA	N	ASSEGNISTA	data analisi	X X X	X X X	X
32	gabriella.delucia	gabriella.delucia@inaf.it	O.A. TRIESTE	Y	PRIMO RICERCATORE	sviluppo modelli	X X X	X X X	X
33	alessandra.derosa	alessandra.derosa@inaf.it	IAPS ROMA	Y	RICERCATORE	data analisi	X X X	X X X	X
34	andrea.comastri	andrea.comastri@inaf.it	OAS BOLOGNA	Y	DIRIGENTE DI RICERCA	coordinamento	X X X	X X X	X
35	chiara.feruglio	chiara.feruglio@inaf.it	O.A. TRIESTE	Y	RICERCATORE	coordinamento e data analisi	X X X	X X X	X
36	angela.bongiorno	angela.bongiorno@inaf.it	O.A. ROMA	Y	RICERCATORE	data analisi	X X X	X X X	X
37	valentina.dodorico	valentina.dodorico@inaf.it	O.A. TRIESTE	Y	RICERCATORE	Analisi dati	X X X	X X X	X
38	paolo.tozzi	paolo.tozzi@inaf.it	O.A. ARCETRI	Y	DIRIGENTE DI RICERCA	Analisi dati X	X X X	X X X	X

16. Personale Associato INAF coinvolto

#	Nome	E-mail	Struttura	TI	Qualifica	Ruolo nel Progetto	FTE Impegnate (2022/2023/2024)	FTE Presunte (2022/2023/2024)	Extra
1	marcella.brusa	marcella.brusa3@unibo.it	Università di Bologna	Y	Professore Associato	Coordinamento	[0.1, 0.1, 0.1]	[0.1, 0.1, 0.1]	0.0
2	stefano.carniani	stefano.carniani@sns.it	Scuola Normale Superiore	Y	Professore Associato	Analisi dati	[0, 0, 0]	[0.0, 0.0, 0.0]	-1.0
3	francesco.tombesi	francesco.tombesi@inaf.it	Università degli Studi di Roma - Tor Vergata	Y	Professore Associato	Analisi dati	[0.2, 0.2, 0]	[-1.0, -1.0, -1.0]	-1.0
4	stefano.bianchi	stefano.bianchi@inaf.it	Università Roma 3	Y	Professore Associato	Coordinamento e analisi dati	[0.1, 0.1, 0]	[-1.0, -1.0, None]	-1.0
5	serafina.digioia	serafina.digioia@inaf.it	Universita' di Trieste	N	Studente Dottorato	Analisi dati	[0, 0, 0]	[0.1, 0.1, 0.0]	-1.0
6	simona.gallerani	simona.gallerani@sns.it	Scuola Normale Superiore di Pisa	Y	Professore associato	Analisi dati	[0.2, 0.2, 0]	[0.0, 0.0, 0.0]	-1.0
7	alessandro.marconi	alessandro.marconi@unifi.it	Universita' di Firenze	Y	Professore Ordinario	Coordinamento	[0, 0, 0]	[0.1, 0.1, 0.1]	-1.0
8	andrea.marinucci	andrea.marinucci@asi.it	ASI	Y	Ricercatore	Coordinamento	[0.1, 0.1, 0]	[-1.0, -1.0, None]	-1.0
9	giorgio.matt	matt@fis.uniroma3.it	Universita' Roma Tre	Y	Professore Ordinario	Modelli	[0.1, 0.1, 0]	[-1.0, -1.0, None]	-1.0
10	simonetta.puccetti	simonetta.puccetti@ssdc.asi.it	ASI	y	Ricercatore	Analisi dati	[0.1, 0.1, 0]	[-1.0, -1.0, None]	-1.0
11	amirnezam.amiri	amirnezam.amiri@inaf.it	Università di Firenze	N	Dottorando	Analisi dati	[0, 0, 0]	[0.0, 0.1, 0.1]	-1.0
12	giulia.tozzi	giulia.tozzi@unifi.it	Università di Firenze	N	Dottoranda di Ricerca	Analisi dati	[0, 0, 0]	[0.0, 0.0, 0.0]	-1.0
13	gabriele.matzeu	gabriele.matzeu@unibo.it	Università di Bologna	N	Assegnista di Ricerca	Analisi dati	[0.2, 0.1, 0]	[0.0, 0.1, 0.1]	-1.0
14	roberta.tripodi	roberta.tripodi@inaf.it	Università di Trieste	N	Studente di dottorato	Analisi dati	[1.0, 1.0, 0]	[-1.0, -1.0, None]	-1.0
15	giacomo.venturi	gventuri@astro.puc.cl	Pontificia Universidad Catolica (Cile)	N	Post-doc	Analisi dati	[0.2, 0.2, 0]	[0.2, 0.2, None]	-1.0
16	michele.perna	michele.perna@cab.inta-csic.es	CAB MAdrid	N	Post-doc	Analisi dati	[0.1, 0.1, 0]	[0.1, 0.1, None]	-1.0
17	fabio.lafranca	fabio.lafranca@uniroma3.it	Universita' Roma3	Y	Professore Ordinario	Analisi dati	[0.1, 0.1, 0]	[0.1, 0.1, -1.0]	-1.0
18	ilaria.ruffa	i.ruffa@ira.inaf.it	Università di Cardiff	N	Ricercatrice post-doc	Analisi dati	[0.2, 0.2, 0]	[0.2, 0.2, None]	-1.0
19	quirino.damato	qdamato@sissa.it	SISSA	N	Postdoc	Analisi dati	[0, 0, 0]	[0.1, 0.1, None]	-1.0
20	federica.ricci	fed.ricci89@gmail.com	Universita' Roma3	N	ricercatore TD A	Analisi dati	[0.6, 0.5, 0]	[0.0, 0.0, 0.0]	-1.0
21	mariavittoria.zanchettin	mariavittoria.zanchettin@studenti.units.it	SISSA	N	Studente Dottorato	Analisi dati	[0.5, 0.5, 0]	[0.2, 0.2, 0.0]	-1.0
22	cristian.vignali	cristian.vignali@unibo.it	Università di Bologna	Y	Professore Associato	Collaboratore	[0, 0, 0]	[0.0, 0.0, 0.0]	-1.0

21. Fondi a Sostegno Iniziativa

PRIN MUR 2017 Black hole winds and the baryon life cycle of galaxies: the stone-guest at the galaxy evolution supper (Ref. F. Fiore) PRIN INAF mainstream 2018 Black hole winds and the baryon cycle (Ref. Fabrizio Fiore) PRIN INAF SKA-CTA 2016 FORECAST (Ref. Isabella Prandoni) ASI-INAF 2017-14-H.0 “Attività di studio di AAE”

Tabella fondi:

#	Provenienza	Certi 2022 (k€)	Certi 2024 (k€)	Presun. 2024 (k€)	Totale Certi (k€)
1	PRIN MUR 2017	100	None	None	100
2	Forecast	0	None	None	0
3	ASI AAE	30	None	None	30

Tabella fondi Astrofisica Fondamentale e PNRR:

#	Provenienza	Fondi 2022 (€)	Fondi 2023 (€)	Fondi 2024 (€)