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PRODID:-//Osservatorio Astrofisico di Catania - ECPv6.14.0//NONSGML v1.0//EN
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X-WR-CALNAME:Osservatorio Astrofisico di Catania
X-ORIGINAL-URL:https://www.oact.inaf.it
X-WR-CALDESC:Eventi per Osservatorio Astrofisico di Catania
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X-PUBLISHED-TTL:PT1H
BEGIN:VTIMEZONE
TZID:UTC
BEGIN:STANDARD
TZOFFSETFROM:+0000
TZOFFSETTO:+0000
TZNAME:UTC
DTSTART:20260101T000000
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=UTC:20260310T113000
DTEND;TZID=UTC:20260310T123000
DTSTAMP:20260404T202822
CREATED:20260309T084132Z
LAST-MODIFIED:20260309T084700Z
UID:19489-1773142200-1773145800@www.oact.inaf.it
SUMMARY:Our Universe in Simulation
DESCRIPTION:Recording: https://www.oact.inaf.it/seminars/ \nDATE: Tuesday\, March 9\, 11:30 a.m. \nORGANIZER: INAF-OACT \nLOCATION: AULA OVEST (INAF-OACT) + remote \nLink for the remote audience:https://meet.google.com/wvf-uwxo-oyj \nSPEAKER: Jia Liu (Kavli IPMU – University of Tokyo) \nABSTRACT:Ongoing and upcoming cosmological surveys—including the Simons Observatory\, LiteBIRD\, Rubin LSST\, Euclid\, DESI\, PSF\, SPHEREx\, and the Roman Space Telescope—will deliver observations of unprecedented precision. Joint analyses across these surveys will be essential for uncovering fundamental physics\, including the nature of inflation\, dark energy\, dark matter\, neutrino mass\, and more. In this talk\, I will discuss the opportunities\, challenges\, and strategies for simulating our universe across multiple wavelengths to realize these goals. \n  \nA few rules:— before joining\, make sure you are using your institutional inaf.it account if you have one (otherwise we will grant you permission to join)— please do not forget to mute your microphone and switch off your webcam when access the virtual room— for questions leave a message in the chat\, the answers at the end of the webinar— the seminar will be recorded\, so if you are interested in it\, please contact us to get the link to the registration. \n 
URL:https://www.oact.inaf.it/event/our-universe-in-simulation/
LOCATION:Sede A. Riccò\, Via Santa Sofia 78\, Catania
CATEGORIES:Eventi & Seminari
ATTACH;FMTTYPE=image/jpeg:https://www.oact.inaf.it/wp-content/uploads/2026/03/seminario_Liu.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260318T080000
DTEND;TZID=UTC:20260417T235900
DTSTAMP:20260404T202823
CREATED:20260318T064229Z
LAST-MODIFIED:20260318T064229Z
UID:19544-1773820800-1776470340@www.oact.inaf.it
SUMMARY:D.D. 59/2026 Concorso pubblico\, per titoli ed esame\, ai fini del reclutamento di una unità di personale con il profilo di "Ricercatore"\, Terzo Livello Professionale\, con contratto di lavoro a tempo determinato e regime di impegno a tempo pieno\, della durata di 12 mesi\, eventualmente prorogabile\, dal titolo “Sviluppo di software per la misura del flusso ottico da mezzo diffuso galattico nei dati Rubin LSST"
DESCRIPTION:Concorso pubblico\, per titoli ed esame\, ai fini del reclutamento di una unità di personale con il profilo di “Ricercatore”\, Terzo Livello Professionale\, con contratto di lavoro a tempo determinato e regime di impegno a tempo pieno\, della durata di 12 mesi\, eventualmente prorogabile\, dal titolo “Sviluppo di software per la misura del flusso ottico da mezzo diffuso galattico nei dati Rubin LSST – Contributo in-kind Rubin Observatory (LOI ITA-INA-S5) (CUP: C83C21000070001 – Ob. Funzione: 1.05.03.06) – Codice bando 2026INAFRIC-OCT-LSST-009\n\nBando
URL:https://www.oact.inaf.it/event/d-d-59-2026-concorso-pubblico-per-titoli-ed-esame-ai-fini-del-reclutamento-di-una-unita-di-personale-con-il-profilo-di-ricercatore-terzo-livello-professionale-con-contratto-di-lavoro-a-tempo/
CATEGORIES:Nuovo,Opportunità di lavoro,Tempo determinato
ATTACH;FMTTYPE=image/jpeg:https://www.oact.inaf.it/wp-content/uploads/2019/06/concorsi_det.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260323T110000
DTEND;TZID=UTC:20260323T123000
DTSTAMP:20260404T202823
CREATED:20260318T081027Z
LAST-MODIFIED:20260318T081030Z
UID:19547-1774263600-1774269000@www.oact.inaf.it
SUMMARY:Magnetic instabilities and angular momentum transport in red giant core
DESCRIPTION:Recording: https://www.oact.inaf.it/seminars/ \nDATE: Monday\, March 23\, 11:00 a.m. \nORGANIZER: INAF-OACT \nLOCATION: AULA OVEST (INAF-OACT) + remote \nLink for the remote audience:https://meet.google.com/wvf-uwxo-oyj \nSPEAKER: Domenico Giovanni Meduri (INAF) \nABSTRACT:The stability of magnetic fields in radiative stellar interiors remains a fundamental open question in understanding the rotational and chemical evolution of low-mass stars. Recent high-resolution asteroseismic observations of red giants have revealed unexpectedly slow core rotations and the presence of strong internal magnetic fields\, opening a new window on the internal dynamics of evolved stars. In this talk\, I will review the main magnetohydrodynamic instabilities expected in radiative stellar interiors and present new 3D direct numerical simulations of the Tayler instability\, a kink-type instability of toroidal magnetic fields prevalent in these regions. By combining simulations\, linear stability analysis\, and stellar evolution models\, we identify where and under what conditions the Tayler instability is likely to operate in red giant cores. These results provide new insight into angular momentum transport in evolved low-mass stars and may also have broader implications for other stars with radiative interiors. \n  \nA few rules:— before joining\, make sure you are using your institutional inaf.it account if you have one (otherwise we will grant you permission to join)— please do not forget to mute your microphone and switch off your webcam when access the virtual room— for questions leave a message in the chat\, the answers at the end of the webinar— the seminar will be recorded\, so if you are interested in it\, please contact us to get the link to the registration. \n 
URL:https://www.oact.inaf.it/event/magnetic-instabilities-and-angular-momentum-transport-in-red-giant-core/
LOCATION:Sede A. Riccò\, Via Santa Sofia 78\, Catania
CATEGORIES:Eventi & Seminari
ATTACH;FMTTYPE=image/jpeg:https://www.oact.inaf.it/wp-content/uploads/2026/03/Meduri_OACT_23mar26_1st_page-0001.jpg
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=UTC:20260403T080000
DTEND;TZID=UTC:20260427T130000
DTSTAMP:20260404T202823
CREATED:20260403T100216Z
LAST-MODIFIED:20260403T100216Z
UID:19582-1775203200-1777294800@www.oact.inaf.it
SUMMARY:D.D. 75/2026 Pubblica selezione per titoli e colloquio per il conferimento di n. 1 borsa di studio\, della durata di 12 mesi\, eventualmente rinnovabile\, dal titolo “Machine learning per l’analisi di segnali in esperimenti fisici e astrofisici con rappresentazioni a grafo”
DESCRIPTION:Pubblica selezione per titoli e colloquio per il conferimento di n. 1 borsa di studio\, della durata di 12 mesi\, eventualmente rinnovabile\, dal titolo “Machine learning per l’analisi di segnali in esperimenti fisici e astrofisici con rappresentazioni a grafo”\, sul Progetto denominato Attività di studio e ricerca per le attività di Calcolo e visualizzazione – Funzione Obiettivo: 2.01.01.03\, CUP C53C22000350006″ \n\nBando\nAllegati
URL:https://www.oact.inaf.it/event/d-d-75-2026-pubblica-selezione-per-titoli-e-colloquio-per-il-conferimento-di-n-1-borsa-di-studio-della-durata-di-12-mesi-eventualmente-rinnovabile-dal-titolo-machine-learning-per-l/
CATEGORIES:Borsa di studio,Nuovo,Opportunità di lavoro
ATTACH;FMTTYPE=image/jpeg:https://www.oact.inaf.it/wp-content/uploads/2019/06/concorsi_borse.jpg
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