Scheda OMAMO FINAL

Informazioni generali

Optomechanical Metrology Alignment and MOnitoring

OMAMO

Programma

R & D

Infrastruttura Inaf

Infrastruttura Internazionale

Attività speciale

RSN5

Attività: In Itinere; Data inizio: 2022; Data fine: 2030

edoardo.redaelli edoardo.redaelli@inaf.it

INAF Brera negli ultimi 10 anni ha sviluppato
tecniche di allineamento di ottiche basato solamente sulla metrologia
meccanica. Questo ha garantito al gruppo un ruolo da leader a livello europeo.
Una grande collaborazione è stata stabilita con l’Europeean souther Observatory
attraverso uno scambio di materiale e personale. Ma anche all’interno dello
stesso INAF. L’obbiettivo ci questa scheda è quello di promuovere le attività
che accresceranno la conoscenza in questo ambito attraverso l’utilizzo di
diverse tecnologie quali i Laser tracker e sistemi di misura interferometrici.

LE SCHEDE INSERITE A PARENTELA DI QUELLA IN OGGETTO SONO PER INDICARE LA TRASVERSALITA' DELL'ATTIVITA' DI RICERCA AI PROGETTI DI INTERESSE INAF

INAF Brera in last 10 years has developed
Optomechanical alignment techniques purely based on mechanical metrology. This
has granted to the team a leading role in the European context. Huge
collaboration has been established with European Southern Observatory by
exchanging of personnel and hardware but also inside INAF among the different
observatories. The aim of this form is to promote the
activities that will increase the expertise in this field using different
technologies like the Laser Tracker and the interferometric measuring system.

THE INSERTED FORM IS RELATED TO THE ONE IN OBJECT INDICATING THE TRASVERSALITY IF THE ACTIVITY WITH RESPECT TO THE MAIN PROJECT OF INAF

Tecnologie per Astronomia Ottica ed Infrarossa

Tecnologie per osservazioni da Terra

Infrastrutture da Terra (utilizzo)

Team Summary

15. Personale INAF coinvolto

Numero di partecipanti INAF al progetto: 15

Struttura	Nfte	TI 2023	TI 2024	TI 2025	TD 2023	TD 2024	TD 2025	Extra
O.A. BRERA	6	0.50	0.50	0.00	0.50	0.50	0.00	0.00
O.A. PADOVA	0	0.00	0.00	0.00	0.00	0.00	0.00	0.00
OAS BOLOGNA	0	0.00	0.00	0.00	0.00	0.00	0.00	0.00
O.A. ARCETRI	0	0.00	0.00	0.00	0	0	0	0.00
O.A. ABRUZZO	0	0	0	0	0.00	0.00	0.00	0.00
Totali	6	0.50	0.50	0.00	0.50	0.50	0.00	0.00

Fondi a sostegno

21. Totale fondi a disposizione (dato aggregato, k€)

Certi 2023	Certi 2024	Certi 2025	Presunti 2023	Presunti 2024	Presunti 2025
715.0	0.0	0.0	0.0	0.0	0.0

Produzione scientifica e tecnologica

22. Produzione scientifica e tecnologica - Highlights

#	DOI	Descrizione
1	https://doi.org/10.1117/12.2563883	Manufacturing, integration, and mechanical verification of SOXS Autori Matteo Aliverti, Luca Oggioni, Matteo Genoni, Giorgio Pariani, Ofir Hershko, Anna Brucalassi, Giuliano Pignata, Hanindyo Kuncarayakti, Ricardo Zanmar Sanchez, Matteo Munari, Sergio Campana, Pietro Schipani, Riccardo Claudi, Andrea Baruffolo, Sagi Ben-Ami, Federico Biondi, Giulio Capasso, Rosario Cosentino, Francesco D'Alessio, Paolo D'Avanzo, Marco Landoni, Adam Rubin, Salvatore Scuderi, Fabrizio Vitali, David Young, Jani Achrén, José Antonio Araiza-Duran, Iair Arcavi, Rachel Bruch, Enrico Cappellaro, Mirko Colapietro, Massimo Della Valle, Marco De Pascale, Rosario Di Benedetto, Sergio D'Orsi, Avishay Gal-Yam, Marcos Hernandez, Jari Kotilainen, Gianluca Li Causi, Seppo Mattila, Michael Rappaport, Kalyan Radhakrishnan, Edoardo Maria Alberto Redaelli, Davide Ricci, Marco Riva, Bernardo Salasnich, Stephen Smartt, Maximilian Stritzinger, Hector Ventura Data pubblicazione 2020/12/28 Conferenza Ground-based and Airborne Instrumentation for Astronomy VIII
2	https://doi.org/10.1117/12.2562129	ESPRESSO fiber-Link upgrade: III-alignment and integration activities Autori Matteo Aliverti, Giorgio Pariani, Gerardo Avila, Luca Oggioni, Edoardo Maria Alberto Redaelli, Marco Riva, Francesco Pepe, Ian Huges, Denis Megèvand, Bruno Chazelas, Felix Garcia Temich, Jose Luis Rasilla The ESPRESSO spectrograph is a high resolution, super stable echelle cross-dispersed fibre-fed spectrograph, installed in the ESO-VLT Combined Coudé Laboratory of the ESO-VLT in Cerro Paranal. In the framework of the Fiber-Link (FL) recovery project, which was necessary to meet the throughput requirement of the instrument, we redesigned and build the whole fibre bundle. The FL subsystem of ESPRESSO is composed by the Input Ends (IE), one per telescope and observing mode, which inject the telescope light into the fibres, the double scrambler and the light combiner for the multi-telescope mode, which merges the light of the four telescopes in a single fibre, and the spectrograph entrance slit. In this paper we focus on the alignment strategy, the tools developed and the activities performed to integrate the different components of the FL
3	https://doi.org/10.1117/1.JATIS.5.1.018005	Simulating the optical alignment of the multiconjugate adaptive optics module for the extremely large telescope Autori Mauro Patti, Matteo Lombini, Edoardo Maria Alberto Redaelli, Emiliano Diolaiti Adaptive optics (AO) instruments for the future extremely large telescopes (ELTs) are characterized by advanced optical systems with diffraction-limited optical quality. Low geometric distortion is also crucial for high accuracy astrometric applications. Optical alignment of such systems is a crucial step of the instrument integration. Due to relative inaccessibility of these giant instruments, automatic alignment methods are also favored to improve the instrument availability after major events, such as extraordinary maintenance. The proposed alignment concept for these systems is described: the notable example which is analyzed here is the case of the multiconjugate AO relay for the future ELT. The results of ray-tracing simulations carried out to validate the method are discussed in detail, covering the error sources, which could degrade the alignment performance.
4	https://doi.org/10.1117/12.2233997	Integration, alignment, and verification of the ESPRESSO Front-End G. Pariani, M. Aliverti, M. Moschetti, M. Landoni, M. Riva, F. M. Zerbi, D. Mégevand, S. Cristiani, F. Pepe ESPRESSO, Echelle SPectrograph for Rocky Exoplanets and Stable Spectroscopic Observations, is now under the assembly, integration and verification phase and will be installed beginning next year at Paranal Observatory on ESO's Very Large Telescopes. The Front End is the modular system in the Combined Coudé Laboratory receiving the light from the four VLT Units, providing the needed connection between the input signal, i.e., object light, sky light, and calibration light, to feed the spectrograph through optical fibers. The modular concept of the FE Units drove the system design and the alignment workflow. We will show the integration method of the single FE modules adopted to guarantee the necessary repeatability between the different Units. The performances of the system in terms of image quality and encircled energy in the observed point spread function are reported. Finally, the strategy followed in the Paranal Combined Coudè Laboratory to define the convergence point of the four UTs is described, along with the procedure used to align the ground plates, the main structure, and the mode selector.
5	https://doi.org/10.1117/12.2561576	SOXS: effects on optical performances due to gravity flexures, temperature variations, and subsystems alignment Ricardo Zanmar Sanchez, Matteo Aliverti, Matteo Munari, Sergio Campana, Riccardo Claudi, Pietro Schipani, Andrea Baruffolo, Sagi Ben-Ami, Federico Biondi, Giulio Capasso, Rosario Cosentino, Francesco D'Alessio, Paolo D'Avanzo, Ofir Hershko, Hanindyo Kuncarayakti, Marco Landoni, Giuliano Pignata, Adam Rubin, Salvatore Scuderi, Fabrizio Vitali, David Young, Jani Achrén, José Antonio Araiza-Duran, Iair Arcavi, Anna Brucalassi, Rachel Bruch, Enrico Cappellaro, Mirko Colapietro, Massimo Della Valle, Marco De Pascale, Rosario Di Benedetto, Sergio D'Orsi, Avishay Gal-Yam, Matteo Genoni, Marcos Hernandez, Jari Kotilainen, Gianluca Li Causi, Seppo Mattila, Michael Rappaport, Kalyan Radhakrishnan, Davide Ricci, Marco Riva, Bernardo Salasnich, Stephen Smartt, Maximilian Stritzinger, Hector Ventura SOXS (Son Of X-Shooter) is the new medium resolution wide-band spectrograph to be installed at the 3.6m New Technology Telescope (NTT) in La Silla. SOXS will offer simultaneous wavelength coverage from 0.35 to 2.0 μm and will be dedicated to the study of transient and variable sources. While nominal optical performances of the system were presented in previous proceedings (Zanmar Sanchez et al. 2018), we here present a set of further analyses aimed to identify and quantify optical effects, due to changes in temperature and orientation of the instrument during alignment and operations.
6	http://hdl.handle.net/20.500.12386/24946	Alignment and integration of large optical systems based on advanced metrology Aliverti, Matteo RIVA, Marco Moschetti, Manuele PARIANI, Giorgio Genoni, Matteo ZERBI, Filippo Maria Optical alignment is a key activity in opto-mechanical system Integration. Traditional techniques require adjustable mounting, driven by optical references that allows the tuning of the optics position along all 6 Degree of Freedom. Nevertheless, the required flexibility imposes reduced stiffness and consequently less stability of the system. The Observatory of Brera (OAB) started few years ago a research activity focused onto the overcoming of this limits exploiting the high metrology performances of Coordinate Measuring Machines (CMM) with the main objectives of relax the manufacturing tolerances and maximize mounting stiffness. Through the T-REX grants, OAB acquired all the instrumentation needed for that activity furthermore considering the ESPRESSO project training and testing also oriented to large scale instrumentation like the E-ELT one. We will present in this paper the definition of the VLTs convergence point and the feasibility study of large mirrors alignment done by mechanical measurements methods.
7	https://doi.org/10.1117/12.2562616	Optomechanical design of MAORY post focal relay optics Edoardo Maria Alberto Redaelli, Matteo Aliverti, Marco Riva, Vincenzo De Caprio, Vincenzo Cianniello, Christian Eredia, Enrico Cascone, Ivan Di Antonio, Mauro Dolci, Gabriele Rodeghiero, Demetrio Magrin, Lorenzo Busoni, Italo Foppiani, Paolo Ciliegi, Ugo Di Giammatteo The different optical designs that locate the optical elements in the MAORY volume impose a different strategy in the design definition of the optomechanics. Considering the different types of elements in the optical design the optomechanics must satisfy the requirement in terms of stiffness, mass and provide a compensating effect respect to the thermal breathing of the materials. In the paper are presented the solutions taken and the mounts working principle. In particular, the aspects that underline and analysed in the simulation are: 1) The behaviour of the mounts in earthquake condition and in thermal survivor condition that means twenty degrees of variation of temperature. 2) The operational condition, the deformation induced in the optical surface due to the gravity, the alignment, and a variation of temperature. 3) The modal analysis of the structure.
8	https://doi.org/10.1117/12.2314460	A possible concept for the day-time calibration and co-phasing of the adaptive M4 mirror at the E-ELT telescope Runa Briguglio, Giorgio Pariani, Marco Xompero, Armando Riccardi, Matteo Tintori, Daniele Gallieni, Roberto Biasi The M4 unit is the deformable mirror providing the E-ELT with adaptive correction of the atmospheric turbulence. The mirror is segmented into 6 petals which are actively shaped by more than 5000 voice-coil actuators. They are controlled in close loop with internal metrology through co-located capacitive position sensors. INAF is involved in the optical calibration and verification of the M4 unit and designed the laboratory optical testbed In this paper, we present a possible auxiliary setup for the mirror calibration once installed at the telescope. The concept implements an on-demand, day-time, optical re-calibration of the mirror, to ensure the years-long term, high accuracy, high precision stability of the internal metrology, beyond the already remarkable intrinsic electronic stability of the M4 unit. The setup exploits the two focii of the quasi-elliptical M3 to create an optical cavity, with the interferometer placed at a Nasmyth focal station of the ELT and a retroreflector (or fiber source) at the M3 short focus to measure the M4 in double (or single) pass. The full monitoring of the M4 optical area allows to: calibrate the actuator influence functions to compute the segments piston tip/tilt commands with high precision; retrieve the flattening command to correct from the low and high order features generated by thermo-mechanical and electrical drifts; compute the phasing command to correct for the segments differential alignment and piston within the requested WF accuracy. The system offers a fast and effective optical maintenance facility for the M4U, without requiring an additional test tower and the mount/dismount down-time of the unit. In this work, we summarize the optical layout and the flattening and segments co-phasing strategy.
9	https://doi.org/10.1117/12.2309951	ELT-HIRES the high resolution spectrograph for the ELT: implementing exoplanet atmosphere reflection detection with a SCAO module Marco Xompero, Christophe Giordano, Marco Bonaglia, Gianluca Di Rico, Guido Agapito, Simone Esposito, Andrea Tozzi, Nicoletta Sanna, Ernesto Oliva, Alessandro Marconi The HIRES-ELT instrument foresees an observing mode that delivers integral field high resolution spectroscopy with spatial sampling down to the diffraction limit of the ELT telescope. The IFU-SCAO module presented here is sub-system of the front-end of HIRES-ELT that includes two modules: SCAO and IFU. The first is the wavefront sensor, based on a pyramid beam-splitter, that provides the guiding on the reference star and the analysis of the incoming wavefront; the second is the module that transforms the incoming f/17.7 light beam from the telescope to the appropriate f/numbers to feed the spectrometer fibers-array with the required spatial scale. In this paper, we will present the SCAO optical design to allow the exoplanet atmosphere detection in reflection. To achieve this goal, we studied a feasible pyramid wavefront sensor to be inserted in a sliding arm of the HIRES front end. The CCD camera is based on a CCD220 chip in which will be imaged the telescope pupil, sampled with a 90x90 sub-aperture grid. A total of 4089 Karhunen-Loeve modes have been generated and used to close an end-to-end simulation. The AO loop runs up to 1000 KHz and it allows to shrink the PSF to the diffraction limits of the telescope ant to achieve Strehl Ratio (SR) above 70% in best seeing case up to magnitude 15 in H-band and a SR permanently above 40%, same band, up to magnitude 14 in case of median seeing. For λ=1600nm the 50% of energy is reached before 1 λ/D for all the plotted I-magnitude under the best seeing conditions. Under Median seeing conditions, the 50% is reached before 2λ/D up to I-mag 13. For λ=1000nm instead, we reach the 50% of encircled energy before a radius of 2λ/D for I-mag less than 14 and after 5λ/D for I-mag greater than 15 in the best seeing case. For each IFU spatial sampling and resolution, we can reach a contrast of 103 at a distance of 4 spaxels from central peak.
10	https://doi.org/10.1117/12.2630064	Titolo: MAORY/MORFEO@ELT: optomechanical preliminary design Autori:Edoardo Maria Alberto Redaelli and Matteo Aliverti and Bortolino Saggin and Jacopo Farinato Publisher:SPIE Anno pubblicazione:2022

Informazioni Pubbliche

<span style="font-size:11pt;font-family:Arial;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;">Le infrastrutture coinvolte sono: <span style="font-size:11pt;font-family:Arial;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;">Gli istituti inaf che si occupano di allineamento:<ul style="margin-top:0;margin-bottom:0;padding-inline-start:48px;"><li dir="ltr" style="list-style-type:disc;font-size:11pt;font-family:Arial;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;" aria-level="1"><span style="font-size:11pt;font-family:Arial;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;">Osservatorio astronomico di Brera</li><li dir="ltr" style="list-style-type:disc;font-size:11pt;font-family:Arial;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;" aria-level="1"><span style="font-size:11pt;font-family:Arial;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;">Osservatorio astronomico di Arcetri</li><li dir="ltr" style="list-style-type:disc;font-size:11pt;font-family:Arial;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;" aria-level="1"><span style="font-size:11pt;font-family:Arial;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;">Osservatorio astronomico  di Padova</li></ul><span style="font-size:11pt;font-family:Arial;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;">Istituti nazionali e internazionali con strette interazioni:<ul style="margin-top:0;margin-bottom:0;padding-inline-start:48px;"><li dir="ltr" style="list-style-type:disc;font-size:11pt;font-family:Arial;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;" aria-level="1"><span style="font-size:11pt;font-family:Arial;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;">European Southern Observatory </li><li dir="ltr" style="list-style-type:disc;font-size:11pt;font-family:Arial;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;" aria-level="1"><span style="font-size:11pt;font-family:Arial;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;">CERN</li><li dir="ltr" style="list-style-type:disc;font-size:11pt;font-family:Arial;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;" aria-level="1"><span style="font-size:11pt;font-family:Arial;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;">Politecnico di Milano</li><li dir="ltr" style="list-style-type:disc;font-size:11pt;font-family:Arial;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;" aria-level="1"><span style="font-size:11pt;font-family:Arial;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;">Large Binocular Telescope</li></ul><span style="font-size:11pt;font-family:Arial;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;">Aziende private<ul style="margin-top:0;margin-bottom:0;padding-inline-start:48px;"><li dir="ltr" style="list-style-type:disc;font-size:11pt;font-family:Arial;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;" aria-level="1"><span style="font-size:11pt;font-family:Arial;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;">ADS</li></ul>

15. Team members, Informazioni generali

15. Personale INAF coinvolto

#	Nome	E-mail	Struttura	TI	Qualifica	Ruolo nel Progetto	FTE Impegnate (2023/2024/2025)	FTE Presunte (2023/2024/2025)	Extra
1	edoardo.redaelli	edoardo.redaelli@inaf.it	O.A. BRERA	N	TECNOLOGO	PI	X X X	X X X	X
2	matteo.aliverti	matteo.aliverti@inaf.it	O.A. BRERA	Y	TECNOLOGO	COPI	X X X	X X X	X
3	luca.oggioni	luca.oggioni@inaf.it	O.A. BRERA	N	TECNOLOGO	AIV expert	X X X	X X X	X
4	matteo.genoni	matteo.genoni@inaf.it	O.A. BRERA	N	TECNOLOGO	AIV expert	X X X	X X X	X
5	giorgio.pariani	giorgio.pariani@inaf.it	O.A. BRERA	Y	TECNOLOGO	AIV expert	X X X	X X X	X
6	marco.riva	marco.riva@inaf.it	O.A. BRERA	Y	PRIMO TECNOLOGO	PM	X X X	X X X	X
7	jacopo.farinato	jacopo.farinato@oapd.inaf.it	O.A. PADOVA	Y	PRIMO TECNOLOGO	AIV expert	X X X	X X X	X
8	luca.marafatto	luca.marafatto@oapd.inaf.it	O.A. PADOVA	Y	TECNOLOGO	AIV expert	X X X	X X X	X
9	gabriele.rodeghiero	gabriele.rodeghiero@inaf.it	OAS BOLOGNA	Y	TECNOLOGO	AIV expert	X X X	X X X	X
10	runa.briguglio	runa.briguglio@inaf.it	O.A. ARCETRI	Y	TECNOLOGO	AIV expert	X X X	X X X	X
11	armando.riccardi	armando.riccardi@inaf.it	O.A. ARCETRI	Y	PRIMO RICERCATORE	AIV expert	X X X	X X X	X
12	luca.rosignoli	luca.rosignoli@inaf.it	OAS BOLOGNA	N	ASSOCIATO - DOTTORANDO STRUTTURE	AIV expert	X X X	X X X	X
13	gabriele.umbriaco	gabriele.umbriaco@unipd.it	O.A. PADOVA	N	ASSOCIATO	AIV expert	X X X	X X X	X
14	carmelo.arcidiacono	carmelo.arcidiacono@inaf.it	O.A. PADOVA	Y	RICERCATORE	AIV expert	X X X	X X X	X
15	benedetta.difrancesco	benedetta.difrancesco@inaf.it	O.A. ABRUZZO	N	ASSEGNISTA	AIV expert	X X X	X X X	X

16. Personale Associato INAF coinvolto

#	Nome	E-mail	Struttura	TI	Qualifica	Ruolo nel Progetto	FTE Impegnate (2023/2024/2025)	FTE Presunte (2023/2024/2025)	Extra

21. Fondi a Sostegno Iniziativa

l'attività di allineamento basata sul Laser Tracker (LT) è stata finanziata ad oggi caricando le spese di sviluppo tecnologico sui vari progetti che hanno beneficiato nella stessa. È stata inserita all'interno del PNRR una richiesta focalizzata sostanzialmente all'acquisizione di nuove macchine per sviluppare al meglio questa stessa attività. L'approvazione del PNRR all'inizi del 2023, permette di acquistare i seguenti dispositivi hardware e software come il LT Leica AT 930, il software Spatial Analyser, e il sistema Multiline di Hexagon. inoltre si aggiungono i fondi vinti con il Minigrant per formazione e acquisto di altra strumentazione come SMR e nest. Lo sviluppo complessivo di fondi Si assesta a 715.000 €

Tabella fondi:

#	Provenienza	Certi 2023 (k€)	Certi 2025 (k€)	Presun. 2025 (k€)	Totale Certi (k€)
1	MAORY	5	None	None	5
2	CUBES	5	None	None	5
3	ANDES	5	None	None	5
4	SOXS	0	None	None	0
5	M4 ELT	5	None	None	5
6	PNRR	675	0	0	675

Tabella fondi Astrofisica Fondamentale e PNRR:

#	Provenienza	Fondi 2023 (€)	Fondi 2024 (€)	Fondi 2025 (€)
1	INAF - Mini Grant	20000.0