Development of a C-band PAF prototype (SKA-4)
SKA-4
Progetto
Programma
R & D
Infrastruttura Internazionale
RSN5
Infrastrutture
Attività: In Itinere; Data inizio: 2017; Data fine: 2024
tonino.pisanu tonino.pisanu@inaf.it
Le survey di grandi aree di cielo con
elevata sensibilità sono uno strumento essenziale per effettuare nuove scoperte
in radioastronomia. Un PAF (Phased Array Feed) posizionato nel piano focale di
un antenna, può aumentare notevolmente il campo di vista e l'efficienza di un
radiotelescopio. In questo programma vogliamo sviluppare un prototipo di PAF in
banda C in cui il beamformer sia basato su schede digitali RFSoC. Il PAF
opererà nel range 4,75 - 6 GHz, utilizzando un sottoinsieme di 32 elementi
collegati agli LNA del totale delle 128 antenne che costituiranno l'array. I 32
segnali verranno poi inviati a 2 schede RFSoC, ognuna delle quali ha 16 canali con
una banda istantanea di 1.25 GHz
High-sensitivity large-scale surveys are an essential tool for new discoveries in radio astronomy. A Phased Array Feed (PAF) placed at the focal plane of an antenna can increase its Field-of-View (FoV) and mapping efficiency. We are developing a prototype of a room-temperature C-band Phased Array Feed (PAF) demonstrator based on Radio Frequency System-on-Chip (RFSoC). The instrument operates across the 4.75-6.00 GHz RF band (C-band). A subset of 32 elements of one of the two polarization channels of the 128 antennas are connected to the LNAs. Following two stages of filtering and signal conditioning, the 32 RF signals are injected in two commercial RFSoC digital boards, each accepting 16 inputs with 1.25 GHz bandwidth that will perform the frequency channelization and the beamforming.
Tecnologie per Astronomia Radio
Tecnologie Informatiche e software
Trasferimento Tecnologico
Struttura | Nfte | N0 | TI 2023 | TI 2024 | TI 2025 | TD 2023 | TD 2024 | TD 2025 | Nex | Extra |
---|---|---|---|---|---|---|---|---|---|---|
O.A. CAGLIARI | 9 | 0 | 0.70 | 0.90 | 0.90 | 0.10 | 0.10 | 0.10 | 1 | 0.20 |
O.A. ARCETRI | 2 | 0 | 0.30 | 0.30 | 0.30 | 0 | 0 | 0 | 0 | 0.00 |
O.A. CATANIA | 2 | 0 | 0.30 | 0.30 | 0.30 | 0 | 0 | 0 | 0 | 0.00 |
Totali | 13 | 0 | 1.30 | 1.50 | 1.50 | 0.10 | 0.10 | 0.10 | 1 | 0.20 |
Certi 2023 | Certi 2024 | Certi 2025 | Presunti 2023 | Presunti 2024 | Presunti 2025 |
---|---|---|---|---|---|
110.0 | 0.0 | 0.0 | 190.0 | 0.0 | 0.0 |
<p class="MsoNormal" style="margin-top:12.0pt;margin-right:0cm;margin-bottom: 12.0pt;margin-left:0cm;text-align:justify"><span lang="EN-GB">Observational Astronomy \ Astronomical detectors \ Radio receivers <o:p></o:p></span></p> <p class="MsoNormal" style="margin-top:12.0pt;margin-right:0cm;margin-bottom: 12.0pt;margin-left:0cm;text-align:justify"><span lang="EN-GB"><a href="http://astrothesaurus.org/uat/1355"><span style="color: windowtext; text-decoration-line: none;">http://astrothesaurus.org/uat/1355</span></a><o:p></o:p></span></p> <p style="margin-top: 0cm; background-image: initial; background-position: initial; background-size: initial; background-repeat: initial; background-attachment: initial; background-origin: initial; background-clip: initial;"><span style="text-align: justify; font-family: var(--bs-font-sans-serif); font-size: 1rem;">Radio astronomy; Radio telescopes; Interferometers; Radio observatories</span><span style="font-family: "Segoe UI", sans-serif; font-size: 1rem;">terferometers; Radio observatories</span><br></p>
<p class="MsoNormal"><span lang="EN-GB">INAF played a fundamental role in the design, development and deployment of the cryogenic C-band phased array feed prototypes for radio astronomy application. Owing to that, INAF now has a recognized role in the field of PAF technologies in the international context. We are also an important component of the RADIOBLOCKS European Project in which the WP3 is almost exclusively devoted to new research for PAF developments.<o:p></o:p></span></p>
<p class="MsoNormal" style="margin-top:12.0pt;margin-right:0cm;margin-bottom: 12.0pt;margin-left:0cm;text-align:justify"><span lang="it">The INAF Observatories contributing to the proposed activities are: Osservatorio Astronomico di Cagliari, the Osservatorio Astrofisico di Arcetri and the Osservatorio Astrofisico di Catania.<o:p></o:p></span></p><p> </p><p class="MsoNormal" style="margin-top:12.0pt;margin-right:0cm;margin-bottom: 12.0pt;margin-left:0cm;text-align:justify"><span lang="EN-US">The principal Scientific infrastructures interested in the project are: SKA, SRT, MeerKAT<b><o:p></o:p></b></span></p>
# | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2023/2024/2025) | FTE Presunte (2023/2024/2025) | Extra | ||
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1 | alessandro.navarrini | alessandro.navarrini@inaf.it | O.A. CAGLIARI | Y | PRIMO TECNOLOGO | Coordinator of system design | X X X | X X X | X | |
2 | pierluigi.ortu | pierluigi.ortu@inaf.it | O.A. CAGLIARI | Y | C.T.E.R. | Monitor and control and bias electronics | X X X | X X X | X | |
3 | tonino.pisanu | tonino.pisanu@inaf.it | O.A. CAGLIARI | Y | TECNOLOGO | System Management of PAF | X X X | X X X | X | |
4 | adelaide.ladu | adelaide.ladu@inaf.it | O.A. CAGLIARI | Y | TECNOLOGO | Design and characterization of RF module | X X X | X X X | X | |
5 | pasqualino.marongiu | pasqualino.marongiu@inaf.it | O.A. CAGLIARI | Y | C.T.E.R. | Mechanical system and cryostat | X X X | X X X | X | |
6 | andrea.melis | andrea.melis@inaf.it | O.A. CAGLIARI | Y | TECNOLOGO | Development of digital beamformer | X X X | X X X | X | |
7 | renzo.nesti | renzo.nesti@inaf.it | O.A. ARCETRI | Y | TECNOLOGO | Electromagnetic design and antenna coupling | X X X | X X X | X | |
8 | giovanni.comoretto | giovanni.comoretto@inaf.it | O.A. ARCETRI | Y | ASTRONOMO ASSOCIATO | Development of digital beamformer | X X X | X X X | X | |
9 | luca.schirru | luca.schirru@inaf.it | O.A. CAGLIARI | Y | TECNOLOGO | Electromagnetic simulations, beam-pattern tests and design and characterization of RF module | X X X | X X X | X | |
10 | paolo.maxia | paolo.maxia@inaf.it | O.A. CAGLIARI | N | TECNOLOGO | Electromagnetic simulations, front end design and development | X X X | X X X | X | |
11 | paola.dininni | paola.dininni@inaf.it | O.A. ARCETRI | Y | TECNOLOGO | Electromagnetic simulations, beam-pattern tests and design and characterization of RF module | X X X | X X X | X | |
12 | massimiliano.belluso | massimiliano.belluso@inaf.it | O.A. CATANIA | Y | C.T.E.R. | Development of digital beamformer/RFSoC | X X X | X X X | X | |
13 | sergio.billotta | sergio.billotta@inaf.it | O.A. CATANIA | Y | TECNOLOGO | Development of digital beamformer/RFSoC | X X X | X X X | X | |
14 | alessandro.cabras | alessandro.cabras@inaf.it | O.A. CAGLIARI | N | ASSEGNISTA | Monitor and control software; | X X X | X X X | X | |
15 | francesco.gaudiomonte | fgaudiom@oa-cagliari.inaf.it | O.A. CAGLIARI | Y | C.T.E.R. | Monitoring and control of the RFI signals and on their impact on the PAF | 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 |
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INAF is part of the SKA Phased Array Feed (PAF) Advanced Instrumentation Program (AIP), which kicked-off in August 26th, 2016 in Cagliari, Italy. Since 2017, PAF activities have been funded by INAF on a yearly basis and conducted by the INAF PAF team in the framework of the SKA PAF AIP. So far, the INAF PAF team has received 365 k€ total funds for the PHAROS2 programme.
# | 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 | 1.05.03.32.02 | 110 | 0 | 0 | 190 | 0 | 0 | 110 | 190 |
# | Provenienza | Fondi 2023 (€) | Fondi 2024 (€) | Fondi 2025 (€) |
---|