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BEGIN:VEVENT
DTSTART;TZID=Atlantic/Canary:20161123T123000
DTEND;TZID=Atlantic/Canary:20161123T133000
UID:iactalks-966
X-WR-CALNAME: IAC Talks: Open Astronomy Seminars
X-ORIGINAL-URL: /iactalks/Talks/view/966
CREATED:2016-11-23T12:30:00+00:00
X-WR-CALDESC: IAC Talks upcomming talks
SUMMARY:Observing with the SARA remotely operated telescopes
DESCRIPTION:Observing with the SARA remotely operated telescopes\nDr. Javie
 r Licandro\n\nThe IAC is part of the&nbsp; Southeastern Association for Re
 search in  Astronomy (SARA), a consortium of colleges and universities in 
 the US  partnered with Lowell Observatory, the Chilean National Telescope 
  Allocation Committee, and the Instituto de Astrofisica de Canarias.  In t
 his seminar I will describe the remote facilities operated by the  SARA ob
 servatories that comprise a 0.96m telescope at Kitt Peak,  Arizona; a 0.6m
  instrument on Cerro Tololo, Chile; and the 1m Jacobus  Kapteyn Telescope 
 at the ORM. All are operated using standard VNC or  Radmin protocols commu
 nicating with on-site PCs. Remote operation offers  considerable flexibili
 ty in scheduling, allowing long-term observational  cadences difficult to 
 achieve with classical observing at remote  facilities. Multiple observers
  at different locations can share a  telescope for training, educational u
 se, or collaborative research  programs. Each telescope has a CCD system f
 or optical imaging, using  thermoelectric cooling to avoid the need for fr
 equent local service, and  a second CCD for offset guiding. SARA Kitt Peak
  telescope also has a  fiber-fed echelle spectrograph. Switching between i
 maging and  spectroscopy is very rapid, so a night can easily accommodate 
 mixed  observing modes.  The IAC astronomers started to use SARA facilitie
 s since early 2016 and  a new call for proposals is open. I will present s
 ome early results from  IAC&rsquo;s observational programs and discuss the
  present status of the  facilities and the experience obtained by the IAC 
 users that could help  new potential observers to prepare their own propos
 als.
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