BEGIN:VCALENDAR VERSION:2.0 PRODID:-//CERN//INDICO//EN BEGIN:VEVENT SUMMARY:Superconducting Nanowire Single Photon Detectors: From Research to Industry DTSTART;VALUE=DATE-TIME:20241219T095500Z DTEND;VALUE=DATE-TIME:20241219T101500Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1406@cern.ch DESCRIPTION:Speakers: chengjun zhang (UNINA)\nSuperconducting nanowire sin gle photon detectors (SNSPDs) are advanced devices renowned for their high sensitivity\, low noise\, and fast speed\, making them ideal for single p hoton detection applications such as quantum communication\, photonic quan tum computing\, imaging\, and LIDAR. Today\, I will share the advanced SNS PD technologies developed by our group and discuss our efforts to transiti on these innovations from research to industry.\n\nhttps://indico.unina.it /event/86/contributions/1406/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1406/ END:VEVENT BEGIN:VEVENT SUMMARY:The PDU test facility for the Darkside20k experiment. DTSTART;VALUE=DATE-TIME:20241218T143000Z DTEND;VALUE=DATE-TIME:20241218T145000Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1388@cern.ch DESCRIPTION:Speakers: Yury Suvorov (UNINA / INFN Sez. Napoli)\nThe DarkSid e-20k is a 20-tonne fiducial mass dual phase Liquid Argon Time Projection Chamber (LArTPC) detector for the direct dark matter search\, filled with low radioactivity Argon and equipped with customised cryogenic SiPM phot osensors. The experiment will be constructed in INFN Gran Sasso undergroun d Laboratory (LNGS)\, and is expected to be free of any instrumental backg round for an exposure of >100 tonne year.\nThe DarkSide SiPMs were develop ed specifically for LAr use in collaboration with Fondazione Bruno Kessler (FBK). This activity leaded to the production and assembly of large surfa ce arrays of SiPMs (20×20 cm2) the Photo Detection Units (PDU) in a INFN dedicated production site NOA at LNGS. The total of 528 PDUs will be prod uced in the following year to be allocated on the two Optical Planes (OP) of the TPC (with ~21 m2 total SiPM surface).\nAll PDUs before installatio n on the OP must be tested and qualified in LN\, this will done in a dedic ated test facility (PDU Test Facility) designed\, assembled and commission ed in Naples Cryogenic Laboratory for the Dark Matter Direct Searches of U NINA Physics Department.\nTwo one-month long testing campaigns with very f irst 6 and later 10 PDUs were conducted in Naples in May and October of 20 24. The PDUs were tested for varying over-voltage values and different rea dout and power configurations. The key parameters like SPE position\, Base line RMS\, signal-to-noise ratio\, Gain and Sensitivity as a function of time were acquired for the stability study. The description of tests and r esults will be presented in this talk.\n\nhttps://indico.unina.it/event/86 /contributions/1388/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1388/ END:VEVENT BEGIN:VEVENT SUMMARY:First data from the prototype of DarkSide-20k in Napoli DTSTART;VALUE=DATE-TIME:20241218T145000Z DTEND;VALUE=DATE-TIME:20241218T151000Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1405@cern.ch DESCRIPTION:Speakers: Dmitrii Rudik (UNINA)\nDarkSide-Proto0 (Proto0) is a n experiment developed within the DarkSide-20k project\, a dark matter dir ect detection experiment that aims to hunt for WIMPs using a two-phase arg on time projection chamber (TPC). In preparation for the future DS-20k exp eriment\, Proto0 focuses on investigating and optimizing the production of the ionization signal (S2) in two-phase argon TPCs and validating many of the novel technologies featured in the DS-20k detector on a smaller scale . To achieve this\, Proto0 is equipped with a compact TPC designed to acco mmodate two PDUs\, the 20x20 cm² SiPM-based photon counters developed for DS-20k. The main feature of the Proto0 detector is its flexible TPC desig n\, with independently moving components during operation. This enables an optimization study of S2 formation in relation to geometrical factors and electrical properties. The results obtained from Proto0’s scientific pr ogram will help fine-tune the DS-20k TPC design and contribute to a broade r understanding of the engineering behind future two-phase experiments. Th e experiment is currently located at the cryogenic laboratory of Unina/INF N Napoli\, where it is collecting data using a specially designed cryogeni c setup\, complete with argon condensation\, recirculation\, and purificat ion loops.\n\nhttps://indico.unina.it/event/86/contributions/1405/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1405/ END:VEVENT BEGIN:VEVENT SUMMARY:AGN variability studies in Naples: toward next generation surveys DTSTART;VALUE=DATE-TIME:20241218T105000Z DTEND;VALUE=DATE-TIME:20241218T111000Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1404@cern.ch DESCRIPTION:Speakers: Maurizio Paolillo (Università di Napoli Federico II )\nI will describe the activity aimed at characterising AGN through their variability in preparation for next generation LSST surveys.\n\nhttps://in dico.unina.it/event/86/contributions/1404/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1404/ END:VEVENT BEGIN:VEVENT SUMMARY:"lo zen e l'arte di accettare gli inviti il più tardi possibile" DTSTART;VALUE=DATE-TIME:20241219T110000Z DTEND;VALUE=DATE-TIME:20241219T112000Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1399@cern.ch DESCRIPTION:Speakers: Pietro Santangelo ()\nSu come ho fatto di tutto per non accettare l'invito del professor Iocco\, non riuscendoci.\n\nhttps:// indico.unina.it/event/86/contributions/1399/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1399/ END:VEVENT BEGIN:VEVENT SUMMARY:The Future of the ex Physics Pavilions of the Mostra d’Oltremare - New Perspectives for Research\, Technology\, and Education DTSTART;VALUE=DATE-TIME:20241219T114000Z DTEND;VALUE=DATE-TIME:20241219T120000Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1398@cern.ch DESCRIPTION:Speakers: Giovanni La Rana (On behalf of the “All’Ombra de l Cervo di Rodi” Association)\nThe Former Physics Pavilions of the Mostr a d’Oltremare house a unique scientific and cultural heritage\, bearing witness to a period of great innovation and intellectual activity. Today\, these historic spaces offer an extraordinary opportunity to become a cata lyst for social and cultural development through the establishment of a Ce nter of Excellence dedicated to innovative scientific and technological re search\, continuous education and training\, as well as dissemination of s cientific knowledge. The restoration and revitalization of these pavilions is the central mission of the "All’Ombra del Cervo di Rodi" Association \, which recently organized a workshop to identify potential research oppo rtunities\, technological advancements\, and educational initiatives that could shape the envisioned Center of Excellence. Starting with a brief his torical overview\, the workshop’s key activities will be presented\, alo ngside preliminary concepts for a feasibility plan aimed at creating a Cen ter of Excellence\, which could be focused on quantum research and impleme ntations\, as well as on continuous education.\n\nhttps://indico.unina.it/ event/86/contributions/1398/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1398/ END:VEVENT BEGIN:VEVENT SUMMARY:Fisica freelance DTSTART;VALUE=DATE-TIME:20241219T104000Z DTEND;VALUE=DATE-TIME:20241219T110000Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1397@cern.ch DESCRIPTION:Speakers: Fernando Gargiulo (Istituto di Scuola Superiore Don Lorenzo Milani\, Gragnano)\nDopo il dottorato in Fisica teorica ed un brev e periodo come Post-doc\, ho sperimentato gli ambienti di lavoro di una st art-up\, di una grande azienda e di una scuola superiore. Finché ho decis o di provare a costruire una carriera come fisico freelance. \nOggi (novem bre 2024) insegno matematica e fisica in un liceo per la metà del tempo\, e faccio il fisico freelance per l'altra metà. \nQuesto talk è duplice. Nella prima parte\, parlerò della fisica computazionale come strumento d idattico per la scuola superiore. Nella seconda\, farò una panoramica del le mia attività come Fisico libero professionista\, con l'auspicio che po ssano ispirare chiunque cerchi attività alternative all'accademia\, alla grande azienda e al sistema scolastico.\n\nhttps://indico.unina.it/event/8 6/contributions/1397/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1397/ END:VEVENT BEGIN:VEVENT SUMMARY:Cosa ho imparato parlando e scrivendo di scienza DTSTART;VALUE=DATE-TIME:20241219T112000Z DTEND;VALUE=DATE-TIME:20241219T114000Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1400@cern.ch DESCRIPTION:Speakers: Giovanni Covone (University Federico II)\nAlcune con siderazioni sulla comunicazione della scienza\, maturate nella mia esperie nza personale tra scuole\, festival\, libri\, tv e teatro.\n\nhttps://indi co.unina.it/event/86/contributions/1400/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1400/ END:VEVENT BEGIN:VEVENT SUMMARY:The Enchantment of Oxygen DTSTART;VALUE=DATE-TIME:20241219T093500Z DTEND;VALUE=DATE-TIME:20241219T095500Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1382@cern.ch DESCRIPTION:Speakers: GABRIELLA MARIA DE LUCA (Diapartimento di Fisica "E . Pancini")\nOxygen\, the lifeblood of all living beings\, is both a bless ing and a challenge for us material physicists working on the materials gr owth for electronics. Superconductivity\, ferroelectricity\, ferromagnetis m\, and multiferroicity—these remarkable properties of materials in oxid es electronics are intrinsically linked to the presence of oxygen. In this presentation\, we will explore how oxygen plays a pivotal role in these p henomena.\n\nhttps://indico.unina.it/event/86/contributions/1382/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1382/ END:VEVENT BEGIN:VEVENT SUMMARY:What quantization means for a mathematician DTSTART;VALUE=DATE-TIME:20241219T091500Z DTEND;VALUE=DATE-TIME:20241219T093500Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1402@cern.ch DESCRIPTION:Speakers: Chiara Esposito (Università di Salerno)\nIn this ta lk I will present the famous Kontsevich Formality theorem\, which solves t he problem of quantization for any Poisson manifolds. Poisson manifolds en codes the information of classical mechanical systems\, while quantum syst ems are encoded by star products. Kontsevich proved that for any Poisson m anifold there exists a star product by proving that we can construct a(n L -infinity) morphism connecting those structures.\n\nhttps://indico.unina.i t/event/86/contributions/1402/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1402/ END:VEVENT BEGIN:VEVENT SUMMARY:Superconducting Nanowires as Targets for Sub-GeV Dark Matter DTSTART;VALUE=DATE-TIME:20241218T141000Z DTEND;VALUE=DATE-TIME:20241218T143000Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1389@cern.ch DESCRIPTION:Speakers: Roberta Calabrese ()\nSuperconducting nanowires repr esent a rapidly developing technology with a broad spectrum of application s in fields such as space communications\, lidar\, and quantum information science. This talk explores the potential of using superconducting nanowi res both as targets and sensors for the direct detection of sub-GeV dark m atter.\nThese devices offer exceptional sensitivity to small energy deposi ts in electrons and demonstrate remarkably low dark count rates\, making t hem ideal for probing electron recoils resulting from dark matter scatteri ng and absorption interactions. We present sensitivity plots for a 4.2 ng NbN device with a dark count rate of $5\\times10^{-4}s^{-1}$ dark count ra te and discuss the projected sensitivities for larger detectors.\n\nhttps: //indico.unina.it/event/86/contributions/1389/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1389/ END:VEVENT BEGIN:VEVENT SUMMARY:Does gravity act on the quantum vacuum? The ARCHIMEDES experiment. DTSTART;VALUE=DATE-TIME:20241218T135000Z DTEND;VALUE=DATE-TIME:20241218T141000Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1387@cern.ch DESCRIPTION:Speakers: LUCIANO ERRICO (Università di Napoli "Federico II" - INFN Sezione di Napoli)\nNel paradigma della Relatività Generale\, l'at trazione gravitazionale è un fenomeno geometrico dello spaziotempo avvert ito tanto dai corpi massivi che dai campi puramente energetici\, come il c ampo elettromagnetico. In quest'ottica\, anche il concetto di peso cambia\ , perchè non dipende solo dalla quantità di materia ma anche dall'energi a interna. Trattandosi di una teoria classica\, si ritiene plausibile l'ef fetto di attrazione sui campi classici\, ma non è ovvio immaginare questo fenomeno sui campi quantistici\, a causa delle divergenze nel calcolo del l'energia di vuoto. \nL'esperimento ARCHIMEDES (INFN - CSN2) si propone di misurare la variazione di peso di un cristallo superconduttivo di BSCCO m entre viene indotta una variazione di energia di vuoto interna dalla trans izione di fase. La variazione di peso attesa è così piccola (0.5 fN) che è stato necessario costruire *ad hoc* una bilancia opto-meccanica di alt a precisione operante presso il futuro SUN Laboratory (Lula\, NU)\, essend o la Sardegna uno dei luoghi con rumore sismico più basso d'Europa. \n\nI n the paradigm of General Relativity (GR)\, gravitational attraction is a geometric phenomenon of spacetime felt by both massive bodies and massless fields\, such as the electromagnetic field. In this context\, the concept of weight also changes\, because it depends not only on the amount of mat ter but also on internal energy. Since GR is a classical theory\, the effe ct of attraction on classical fields is considered plausible\, but it is n ot obvious to imagine this phenomenon on quantum fields\, due to divergenc es in the calculation of vacuum energy. The ARCHIMEDES experiment (INFN - CSN2) aims to measure the weight change of a superconducting BSCCO crystal while an internal vacuum energy variation is induced by the phase transit ion. The expected weight variation is so small (0.5 fN) that a high-precis ion opto-mechanical balance had to be built *ad hoc* at the future SUN Lab oratory (Lula\, NU)\, Sardinia being one of the places with the lowest sei smic noise in Europe.\n\nhttps://indico.unina.it/event/86/contributions/13 87/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1387/ END:VEVENT BEGIN:VEVENT SUMMARY:Learning Universe with Artificial Intelligence DTSTART;VALUE=DATE-TIME:20241218T133000Z DTEND;VALUE=DATE-TIME:20241218T135000Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1385@cern.ch DESCRIPTION:Speakers: Nicola R. Napolitano (UniNA )\nI will present a proj ect collecting machine learning tools to extract physical parameters from the major sky surveys and predict the cosmological parameters using millio n to billion galaxy samples.\n\nhttps://indico.unina.it/event/86/contribut ions/1385/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1385/ END:VEVENT BEGIN:VEVENT SUMMARY:Stories of Statistical Physics and Computational Biology DTSTART;VALUE=DATE-TIME:20241218T101000Z DTEND;VALUE=DATE-TIME:20241218T103000Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1395@cern.ch DESCRIPTION:Speakers: Andrea Maria Chiariello (Dipartimento di Fisica Etto re Pancini\, Università di Napoli Federico II)\nWithin the cell nucleus o f eukaryotic organisms\, chromosomes are organized in a complex\, non-rand om three-dimensional (3D) spatial structure\, which is intimately linked t o vital functional purposes. Indeed\, a correct folding allows an efficien t communication between genes and their distal regulatory elements while\, if altered\, can cause severe diseases. Here I will discuss how Polymer P hysics\, combined with Molecular Dynamics simulations and Machine Learning based inference\, represent a powerful tool to quantitatively investigate the complexity of 3D organization of real genomes\, as highlighted by rec ent microscopy and biochemical experiments. I will show that simple physic al processes\, widely studied in Statistical Mechanics\, such as phase-sep aration of molecular aggregates and symmetry breaking mechanisms\, allow u s to make sense of recent experimental observations including the in olfac tory receptor choice in olfactory sensory neurons (OSN). Finally\, polymer models can be used to study the impact of disease-linked genetic mutation s or the effect of viral infections as SARS-CoV-2\, opening the way to new potential tools in Biomedicine.\n\nhttps://indico.unina.it/event/86/contr ibutions/1395/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1395/ END:VEVENT BEGIN:VEVENT SUMMARY:Epidemic Dynamics in Interconnected Populations: Scaling and Polic y Implications DTSTART;VALUE=DATE-TIME:20241218T093000Z DTEND;VALUE=DATE-TIME:20241218T095000Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1393@cern.ch DESCRIPTION:Speakers: Antonio Scala (CNR)\nUnderstanding the dynamics of i nfectious disease spread in interconnected populations is crucial for effe ctive public health planning. In our increasingly mobile world\, tradition al modeling approaches often fall short in capturing the complexities of d isease transmission across vast distances. This paper presents an innovati ve framework that combines the conceptual simplicity of ordinary different ial equations (ODEs) with the predictive capabilities of computational mod els to analyze epidemic dynamics on interconnected networks. We derive sca ling laws for epidemic propagation delays using perturbation expansion tec hniques\, highlighting the influence of network topology and migration flu x. Our findings reveal the diminishing returns of mobility reduction polic ies in mitigating epidemic spread\, particularly after the outbreak has se ttled. This work contributes to a deeper understanding of the mechanisms d riving infectious disease dynamics\, providing quantitative insights for p ublic health authorities to assess risks and optimize response strategies. \n\nhttps://indico.unina.it/event/86/contributions/1393/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1393/ END:VEVENT BEGIN:VEVENT SUMMARY:Modeling the human genome through polymer physics DTSTART;VALUE=DATE-TIME:20241218T091000Z DTEND;VALUE=DATE-TIME:20241218T093000Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1394@cern.ch DESCRIPTION:Speakers: Mattia Conte (Università di Napoli Federico II & IN FN)\nIn the nucleus of cells\, chromosomes have been discovered to self-or ganize into a complex spatial architecture that serves vital functional pu rposes as\, for instance\, genes have to establish specific physical conta cts with their distal DNA regulators to control transcriptional activities . However\, how the system self-assembles to shape the folding of our geno me and its functions is only poorly understood. In this talk\, I discuss p rincipled models of interacting polymers from statistical mechanics to inv estigate the mechanisms whereby distal DNA sequences recognise and interac t with each other. Those theories are validated against independent experi ments\, opening to new tools for real-world applications\, such as the pre diction of the effects of disease-associated mutations\, linked to congeni tal disorders or cancer\, on genome 3D structure.\n\nhttps://indico.unina. it/event/86/contributions/1394/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1394/ END:VEVENT BEGIN:VEVENT SUMMARY:Predictive polymer models of genome 3D structure DTSTART;VALUE=DATE-TIME:20241218T095000Z DTEND;VALUE=DATE-TIME:20241218T101000Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1396@cern.ch DESCRIPTION:Speakers: Simona Bianco ()\nChromosomes have a complex spatia l structure that serves vital functional purposes\, yet their self-organiz ation principles are largely unknown. I discuss our recent work combining polymer physics and machine learning to understand how chromosomes are fol ded and regulated in the cell nucleus. After a brief overview of recent ex perimental advances to measure chromosome 3D structure\, I discuss our phy sics models showing that phase transition mechanisms can control chromosom e architecture and its link with gene regulation and cell function. Severa l experiments have confirmed those models\, notably their predictions on h ow genetic mutations result in diseases such as congenital disorders\, ope ning the way to novel applications in biomedicine.\n\nhttps://indico.unina .it/event/86/contributions/1396/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1396/ END:VEVENT BEGIN:VEVENT SUMMARY:Searching for TeV-emitting candidates among the X-ray bright blaza r population DTSTART;VALUE=DATE-TIME:20241218T111000Z DTEND;VALUE=DATE-TIME:20241218T113000Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1384@cern.ch DESCRIPTION:Speakers: ANTONIO IULIANO (INFN Sezione di Napoli)\nThe purpos e of this work is to understand if\, among the blazars not detected by Fer mi-LAT\, a population of TeV emitting sources could be detected by current or future Cherenkov telescopes. We cross-matched the 5BZCAT catalog of bl azars with the most recent catalogs of point-like source\, to determine i f the X-ray emission can be used as an effective proxy to find and charact erize candidate TeV-emitting blazars.\n\nhttps://indico.unina.it/event/86/ contributions/1384/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1384/ END:VEVENT BEGIN:VEVENT SUMMARY:(No) exotic monsters in the early Universe DTSTART;VALUE=DATE-TIME:20241218T115000Z DTEND;VALUE=DATE-TIME:20241218T121000Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1386@cern.ch DESCRIPTION:Speakers: FABIO IOCCO (Università di Napoli "Federico II")\nT he recent data by the JWST satellite identify what seems an excess of lumi nous objects in the early Universe. It has been proposed that this may be evidence that exotic monsters lurk in the cosmic Dark Ages.\nI will show h ow -while such excesses seems to be consistent and real- they can not be e xplained by some of the most extreme versions of "dark matter supported st ellar objects" that myself and others postulated in the past\, contrary to the claims in this sense.\n\nhttps://indico.unina.it/event/86/contributio ns/1386/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1386/ END:VEVENT BEGIN:VEVENT SUMMARY:JWST and the high redshift Universe DTSTART;VALUE=DATE-TIME:20241218T113000Z DTEND;VALUE=DATE-TIME:20241218T115000Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1383@cern.ch DESCRIPTION:Speakers: Marianna Annunziatella ()\nI will talk about the rec ent discoveries on high redshift galaxies made by JWST in the last year\, and what we can expect from the next rounds of observations.\n\nhttps://in dico.unina.it/event/86/contributions/1383/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1383/ END:VEVENT BEGIN:VEVENT SUMMARY:Welcome and introduction DTSTART;VALUE=DATE-TIME:20241218T090000Z DTEND;VALUE=DATE-TIME:20241218T091000Z DTSTAMP;VALUE=DATE-TIME:20260608T023055Z UID:indico-contribution-86-1392@cern.ch DESCRIPTION:https://indico.unina.it/event/86/contributions/1392/ LOCATION:Dipartimento di Fisica "Ettore Pancini" Aula Caianiello URL:https://indico.unina.it/event/86/contributions/1392/ END:VEVENT END:VCALENDAR