Scheda RADIOQSO
FINAL
Informazioni generali
RADIO EMISSION AND WINDS FEEDBACK IN QUASARS
RADIOQSO
Progetto
RSN4
RSN1
Attività: In Itinere; Data inizio: 2019; Data fine: 2033
francesca.panessa francesca.panessa@inaf.it
Il presente progetto si propone di studiare la natura dell'emissione in banda radio in quasar di tipo Radio-Quiet (RQ). Il principale obiettivo scientifico riguarda la determinazione della prevalenza di emissione radio attribuita a getti, formazione stellare oppure shocks in venti/outlfows. La combinazione di dati in multi-frequenza (attraverso una estensiva campagna osservativa) per campioni di QSO ci consentirà di stabilire la rilevanza dei getti radio nel quasar feedback.
This project aims at determining the morphology and physical nature of radio emission in
RQ quasars. Our objective is to assess the prevalence of radio emission attributed to jets,
star formation, or outflow-driven shocks within quasars. Combined with the multi-phase gas
observations (employing multiple telescopes) from our QSO samples, we want to establish
the relevance of radio jets to quasar feedback as the driver mechanism of gas outflows.
Galassie, AGN e loro evoluzione
Fisica degli oggetti compatti galattici ed extragalattici
Team Summary
15. Personale INAF coinvolto
Numero di partecipanti INAF al progetto: 7
| Struttura | Nfte | N0 | TI 2024 | TI 2025 | TI 2026 | TD 2024 | TD 2025 | TD 2026 | Nex | Extra |
|---|---|---|---|---|---|---|---|---|---|---|
| IAPS ROMA | 1 | 0 | 0.00 | 0.10 | 0.30 | 0.00 | 0.00 | 0.00 | 0 | 0.00 |
| OAS BOLOGNA | 0 | 0 | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 0 | 0.00 |
| IRA BOLOGNA | 0 | 0 | 0 | 0 | 0 | 0.00 | 0.00 | 0.00 | 0 | 0.00 |
| O.A. ROMA | 0 | 0 | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 0 | 0.00 |
| O.A. TRIESTE | 0 | 0 | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 0 | 0.00 |
| Totali | 1 | 0 | 0.00 | 0.10 | 0.30 | 0.00 | 0.00 | 0.00 | 0 | 0.00 |
16. Personale Associato INAF coinvolto
Numero di partecipanti Associati INAF: 4
| # | Struttura | TI 2024 | TI 2025 | TI 2026 | TD 2024 | TD 2025 | TD 2026 | Extra |
|---|---|---|---|---|---|---|---|---|
| 1 | Università di Bologna | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 0.00 |
| 2 | ESAC | 0 | 0 | 0 | 0.20 | 0.20 | 0.20 | 0.00 |
| 3 | Università di Roma Tre | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 0.00 |
| 4 | Università di Firenze | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 0.20 |
| Totali | 0.00 | 0.00 | 0.00 | 0.20 | 0.20 | 0.20 | 0.20 |
Fondi a sostegno
21. Totale fondi a disposizione (dato aggregato, k€)
| Certi 2024 | Certi 2025 | Certi 2026 | Presunti 2024 | Presunti 2025 | Presunti 2026 |
|---|---|---|---|---|---|
| 0 | 0 | 0 | 0 | 0 | 0 |
Produzione scientifica e tecnologica
22. Produzione scientifica e tecnologica - Highlights
Informazioni Pubbliche
<ul><li class="uat"><a href="https://uat.astrothesaurus.org/uat/1447?view=hierarchy">Seyfert galaxies</a></li><li class="uat"><a href="https://uat.astrothesaurus.org/uat/159?view=hierarchy">Black hole physics</a></li><li class="uat"><a href="https://uat.astrothesaurus.org/uat/16?view=hierarchy">Active galactic nuclei</a></li><li class="uat"><a href="https://uat.astrothesaurus.org/uat/162?view=hierarchy">Black holes</a></li><li class="uat"><a href="https://uat.astrothesaurus.org/uat/870?view=hierarchy">Jets</a><a href="https://uat.astrothesaurus.org/uat/1786?view=hierarchy"></a></li></ul><p></p>
<p><span style="font-size:11pt;font-family:Arial,sans-serif;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;" id="docs-internal-guid-0eaf21d2-7fff-10d4-9a54-627b532d062d">The core team is composed of Italian researchers which are leading experts in the field (mostly from INAF). </span><span style="font-size:11pt;font-family:Arial,sans-serif;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;" id="docs-internal-guid-0eaf21d2-7fff-10d4-9a54-627b532d062d"><br></span><span style="font-size:11pt;font-family:Arial,sans-serif;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">Our team is producing a large number of high level scientific papers in the main scientific journals. The Italian astronomical community has committed significant resources to the development of ground-based and space observatories. Our research makes extensive use of state-of-the-art technologies, most of which are fully developed in Europe. Moreover, this project exploits and produces preparatory science for facilities in which INAF has a leading role, such as the European VLBI, LOFAR, the Square Kilometer Array (SKA) and its precursors, Theseus and Athena. These projects are involving several industries in the process of developing/building/testing new technologies, thus boosting several of the Italian industrial capabilities in key enabling technologies.</span></p><br><p></p>
<p dir="ltr" style="line-height:1.38;text-align: justify;margin-top:0pt;margin-bottom:0pt;" id="docs-internal-guid-8e62c69b-7fff-449b-659e-99bd85692908"><span style="font-size:11pt;font-family:Arial,sans-serif;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">Radio astronomy is witnessing a golden age owing to the large number of already available</span></p><p dir="ltr" style="line-height:1.38;text-align: justify;margin-top:0pt;margin-bottom:0pt;"><span style="font-size:11pt;font-family:Arial,sans-serif;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">interferometers and to the high throughput of present and upcoming new facilities (that is,</span></p><p dir="ltr" style="line-height:1.38;text-align: justify;margin-top:0pt;margin-bottom:0pt;"><span style="font-size:11pt;font-family:Arial,sans-serif;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">LOw Frequency ARray (LOFAR), Square Kilometre Array (SKA), new-generation Very Large</span></p><p dir="ltr" style="line-height:1.38;text-align: justify;margin-top:0pt;margin-bottom:0pt;"><span style="font-size:11pt;font-family:Arial,sans-serif;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">Array (ngVLA), Event Horizon Telescope (EHT), ALMA, space VLBI) that will revolutionize</span></p><p dir="ltr" style="line-height:1.38;text-align: justify;margin-top:0pt;margin-bottom:0pt;"><span style="font-size:11pt;font-family:Arial,sans-serif;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">this field. The project involves multi-frequency data obtain worldwide.</span></p><p></p>
15. Team members, Informazioni generali
15. Personale INAF coinvolto
| # | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2024/2025/2026) | FTE Presunte (2024/2025/2026) | Extra | ||
|---|---|---|---|---|---|---|---|---|---|---|
| 1 | francesca.panessa | francesca.panessa@inaf.it | IAPS ROMA | Y | PRIMO RICERCATORE | Coordinatrice | X X X | X X X | X |
|
| 2 | giorgio.lanzuisi | giorgio.lanzuisi@inaf.it | OAS BOLOGNA | Y | PRIMO RICERCATORE | X-ray and multi-frequency data analysis and interpretation | X X X | X X X | X |
|
| 3 | gabriele.bruni | gabriele.bruni@inaf.it | IAPS ROMA | N | RICERCATORE | Radio data analysis and interpretation | X X X | X X X | X |
|
| 4 | marisa.brienza | marisa.brienza@inaf.it | IRA BOLOGNA | N | RICERCATORE | Radio data analysis and interpretation | X X X | X X X | X |
|
| 5 | enrico.piconcelli | enrico.piconcelli@inaf.it | O.A. ROMA | Y | PRIMO RICERCATORE | X-ray and multi-frequency data analysis and interpretation | X X X | X X X | X |
|
| 6 | luca.zappacosta | luca.zappacosta@inaf.it | O.A. ROMA | Y | RICERCATORE | X-ray and multi-frequency data analysis and interpretation | X X X | X X X | X |
|
| 7 | chiara.feruglio | chiara.feruglio@inaf.it | O.A. TRIESTE | Y | PRIMO RICERCATORE | Multiwavelength data interpretation | X X X | X X X | X |
|
16. Personale Associato INAF coinvolto
| # | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2024/2025/2026) | FTE Presunte (2024/2025/2026) | Extra | |
|---|---|---|---|---|---|---|---|---|---|
| 1 | marcella.brusa | marcella.brusa3@unibo.it | Università di Bologna | Y | professoressa associata | Multiwavelength data interpretation | [0, 0, 0] | [0.0, 0.0, 0.0] | 0.0 |
| 2 | gabriele.matzeu | gabriele.matzeu@ext.esa.int | ESAC | N | Ricercatore | X-ray and multi-frequency data analysis and interpretation | [0.2, 0.2, 0.2] | [0.0, 0.0, 0.0] | 0.0 |
| 3 | stefano.bianchi@uniroma3.it | stefano.bianchi@uniroma3.it | Università di Roma Tre | Y | Professoressa Ordinario | X-ray and multi-frequency data analysis and interpretation | [0, 0, 0] | [0.0, 0.0, 0.0] | 0.0 |
| 4 | alessandro.marconi@unifi.it | alessandro.marconi@unifi.it | Università di Firenze | Y | Professore Ordinario | Multiwavelength data interpretation and theory | [0, 0, 0] | [0.0, 0.0, 0.0] | 0.2 |
21. Fondi a Sostegno Iniziativa
Non ci sono fondi su questo progetto
Tabella fondi:
| # | 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€) |
|---|
Tabella fondi Astrofisica Fondamentale e PNRR:
| # | Provenienza | Fondi 2024 (€) | Fondi 2025 (€) | Fondi 2026 (€) |
|---|