BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//Osservatorio Astronomico di Roma - ECPv6.15.18//NONSGML v1.0//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
X-ORIGINAL-URL:https://www.oa-roma.inaf.it
X-WR-CALDESC:Eventi per Osservatorio Astronomico di Roma
REFRESH-INTERVAL;VALUE=DURATION:PT1H
X-Robots-Tag:noindex
X-PUBLISHED-TTL:PT1H
BEGIN:VTIMEZONE
TZID:Europe/Rome
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20230326T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20231029T010000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20240331T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20241027T010000
END:STANDARD
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20250330T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20251026T010000
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20240206T113000
DTEND;TZID=Europe/Rome:20240206T170000
DTSTAMP:20260406T153522
CREATED:20231212T055019Z
LAST-MODIFIED:20240202T164246Z
UID:13270-1707219000-1707238800@www.oa-roma.inaf.it
SUMMARY:colloquium Paolo Saracco - SHARP - A Near-IR Multi-mode Spectrograph conceived for the Multi-Conjugate adaptive optics module MORFEO@ELT
DESCRIPTION:The world’s largest aperture combined with state-of-the-art Adaptive Optics systems will enable the ELT to capture better data than the JWST in both sharpness and depth. Therefore\, the spectrograph intended for the 2nd port of the Multi-Conjugate Adaptive Optics (MCAO) system MORFEO@ELT will be the most powerful instrument of the JWST era\, revealing phenomena beyond the reach of others. SHARP (http://sharp.brera.inaf.it) is a near-IR (0.95-2.45 mu) spectrograph designed for the 2nd port of MORFEO@ELT\, intended to be submitted in the upcoming ESO instrument call. Comprising a Multi-Object Spectrograph\, NEXUS\, and a multi-Integral Field Unit\, VESPER\, SHARP extends its wavelength range to ~2.45 μ. Coupled with MCAO-assisted observations\, it delivers unprecedented high angular (~30 mas) and spectral resolution\, outperforming NIRSpec@JWST (100 mas). MORFEO-SHARP will allow us to study the nearby and the early Universe in unprecedented detail\, resolving the first galaxies and the star forming regions within galaxies far back in cosmic time\, and providing spectra of individual nearby young stellar objects. This presentation introduces the scientific rationale behind SHARP\, showcasing its features and inviting those interested to join the SHARP team.
URL:https://www.oa-roma.inaf.it/event/colloquium-paolo-saracco/
LOCATION:Aula Gratton
CATEGORIES:Seminari
END:VEVENT
END:VCALENDAR