BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//ZContent.net//ZapCalLib 1.0//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
BEGIN:VEVENT
DTSTART;TZID=Atlantic/Canary:20140424T103000
DTEND;TZID=Atlantic/Canary:20140424T113000
UID:iactalks-638
X-WR-CALNAME: IAC Talks: Open Astronomy Seminars
X-ORIGINAL-URL: /iactalks/Talks/view/638
CREATED:2014-04-24T10:30:00+01:00
X-WR-CALDESC: IAC Talks upcomming talks
SUMMARY:MUSE a new instrument at Paranal
DESCRIPTION:MUSE a new instrument at Paranal\nMr. Antonio Manescau\n\nMUSE 
 (Multi Unit Spectroscopic Explorer) is a         2nd generation Integral F
 ield facility for the VLT. With a field         of view of 1x1 arcmin, fin
 e sampling, intermediate spectral         resolution and large spectral co
 verage in the visible, it uses a         complex image slicer, twenty-four
  parallel spectrographs and a         large detector area. In addition, MU
 SE is conceived to work         assisted by the Adaptive Optics Facility (
 AOF), which will         enhance notably its performance. MUSE is the resu
 lt of ten years         of design and development by the MUSE consortium &
 mdash; headed by the         Centre de Recherche Astrophysique de Lyon, Fr
 ance and the         partner institutes Leibniz-Institut f&uuml;r Astrophy
 sik Potsdam         (AIP, Germany),&nbsp; Institut f&uuml;r Astrophysik G&
 ouml;ttingen (IAG,         Germany),&nbsp; Institute for Astronomy ETH Zur
 ich (Switzerland),         L'Institut de Recherche en Astrophysique et Pla
 n&eacute;tologie (IRAP,         France), Nederlandse Onderzoekschool voor 
 de Astronomie (NOVA,         the Netherlands) and ESO. MUSE has been succe
 ssfully installed on ESO&rsquo;s Very Large         Telescope (VLT). In th
 is talk it will be presented the         instrument, its design and challe
 nges, the integration (both in         Europe and Paranal), the first ligh
 t and first commissioning         results.
END:VEVENT
END:VCALENDAR
