BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//ZContent.net//ZapCalLib 1.0//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
BEGIN:VEVENT
DTSTART;TZID=Atlantic/Canary:20230228T123000
DTEND;TZID=Atlantic/Canary:20230228T133000
UID:iactalks-1647
X-WR-CALNAME: IAC Talks: Open Astronomy Seminars
X-ORIGINAL-URL: /iactalks/Talks/view/1647
CREATED:2023-02-28T12:30:00+00:00
X-WR-CALDESC: IAC Talks upcomming talks
SUMMARY:Preparing for MAAT@GTC: pipeline development for the new OSIRIS+ de
 tector
DESCRIPTION:Preparing for MAAT@GTC: pipeline development for the new OSIRIS
 + detector\nDr. David Jones\n\nMAAT is a mirror-slicer integral field unit
  that will be installed in  OSIRIS in 2024, breathing new life into the GT
 C's work horse instrument.  As well as the opportunity to perform spatiall
 y-resolved spectroscopy  over a field of 10"x7", MAAT will also offer incr
 eased signal-to-noise  and resolution for point sources with respect to th
 e standard long slit  mode.  As part of the preparations for the arri
 val of MAAT, we have  implemented support for the reduction of OSIRIS data
  into the  open-source, python-based spectroscopic reduction package PypeI
 t.  Indeed, with the arrival of the new blue-sensitive CCD, PypeIt is now 
  the only publicly available pipeline that continues to work for OSIRIS.  
 With very little human intervention, PypeIt produces fully calibrated  and
  coadded spectra that are near the Poisson limit for point sources.  In th
 is talk, I will present a brief overview of the philosophy behind  PypeIt 
 and demonstrate the ease with which OSIRIS data (and soon MAAT  data) can 
 be reduced.\n 
END:VEVENT
END:VCALENDAR