BEGIN:VCALENDAR
VERSION:2.0
PRODID:IEEE vTools.Events//EN
CALSCALE:GREGORIAN
BEGIN:VTIMEZONE
TZID:Poland
BEGIN:DAYLIGHT
DTSTART:20180325T030000
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
RRULE:FREQ=YEARLY;BYDAY=-1SU;BYMONTH=3
TZNAME:CEST
END:DAYLIGHT
BEGIN:STANDARD
DTSTART:20181028T020000
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
RRULE:FREQ=YEARLY;BYDAY=-1SU;BYMONTH=10
TZNAME:CET
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTAMP:20181031T100736Z
UID:BCC1A721-86E6-4C45-840F-9FE65224CD5A
DTSTART;TZID=Poland:20181026T141500
DTEND;TZID=Poland:20181026T151500
DESCRIPTION:Space is filled of photons of all wavelengths\, from very short
  (e.g.\, gamma) to very long (e.g.\, radio)\, which convey information abo
 ut the processes that generated them. Radio telescopes are used to sense t
 hese lower frequencies in an effort to answer fundamental questions about 
 the composition and evolution of our universe\, further our understanding 
 of physics\, and also to answer the age-old question: “Are We Alone?”\
 n\nAdvances in computing have enabled changes in the paradigms in radio as
 tronomy since the first large single-dish systems\; modern systems can now
  have hundreds\, or thousands\, of antennas\, across geographically-large 
 apertures and linked through signal processing. In this talk\, Dr. Billy B
 arott will present an overview of this subject\, including the science tha
 t motivates these instruments\, and will discuss details of the Allen Tele
 scope Array in particular\, including both engineering details and a sampl
 ing of some experiments that have been performed with this radio telescope
 .\n\nSpeaker(s): William C. Barott\, \n\nRoom: 229\, Bldg: Faculty of Elec
 tronics and Information Technology\, Nowowiejska 15/19\, Warszawa\, Mazowi
 eckie\, Poland\, 00-665
LOCATION:Room: 229\, Bldg: Faculty of Electronics and Information Technolog
 y\, Nowowiejska 15/19\, Warszawa\, Mazowieckie\, Poland\, 00-665
ORGANIZER:psamczyn@elka.pw.edu.pl
SEQUENCE:5
SUMMARY:Exploring the dynamic universe with radio astronomy - Beamforming\,
  Transients\, SETI\, and the Allen Telescope Array
URL;VALUE=URI:https://events.vtools.ieee.org/m/177251
X-ALT-DESC:Description: &lt;br /&gt;&lt;p style=&quot;margin: 0px 0px 10.66px\; text-alig
 n: justify\;&quot;&gt;&lt;span lang=&quot;EN-US&quot; style=&quot;margin: 0px\; color: #222222\; lin
 e-height: 107%\; font-family: &#39;Cambria&#39;\,serif\; font-size: 10pt\;&quot;&gt;Space 
 is filled of photons of all wavelengths\, from very short (e.g.\, gamma) t
 o very long (e.g.\, radio)\, which convey information about the processes 
 that generated them. Radio telescopes are used to sense these lower freque
 ncies in an effort to answer fundamental questions about the composition a
 nd evolution of our universe\, further our understanding of physics\, and 
 also to answer the age-old question: &amp;ldquo\;Are We Alone?&amp;rdquo\;&lt;/span&gt;&lt;
 /p&gt;\n&lt;p style=&quot;margin: 0px 0px 10.66px\; text-align: justify\;&quot;&gt;&lt;span lang
 =&quot;EN-US&quot; style=&quot;margin: 0px\; color: #222222\; line-height: 107%\; font-fa
 mily: &#39;Cambria&#39;\,serif\; font-size: 10pt\;&quot;&gt;Advances in computing have ena
 bled changes in the paradigms in radio astronomy since the first large sin
 gle-dish systems\; modern systems can now have hundreds\, or thousands\, o
 f antennas\, across geographically-large apertures and linked through sign
 al processing. In this talk\, Dr. Billy Barott will present an overview of
  this subject\, including the science that motivates these instruments\, a
 nd will discuss details of the Allen Telescope Array in particular\, inclu
 ding both engineering details and a sampling of some experiments that have
  been performed with this radio telescope.&lt;/span&gt;&lt;/p&gt;
END:VEVENT
END:VCALENDAR

