BEGIN:VCALENDAR
PRODID:-//Microsoft Corporation//Outlook 14.0 MIMEDIR//EN
VERSION:2.0
METHOD:PUBLISH
X-MS-OLK-FORCEINSPECTOROPEN:TRUE
BEGIN:VTIMEZONE
TZID:Pacific Standard Time
BEGIN:STANDARD
DTSTART:16011104T020000
RRULE:FREQ=YEARLY;BYDAY=1SU;BYMONTH=11
TZOFFSETFROM:-0700
TZOFFSETTO:-0800
END:STANDARD
BEGIN:DAYLIGHT
DTSTART:16010311T020000
RRULE:FREQ=YEARLY;BYDAY=2SU;BYMONTH=3
TZOFFSETFROM:-0800
TZOFFSETTO:-0700
END:DAYLIGHT
END:VTIMEZONE
BEGIN:VEVENT
CLASS:PUBLIC
CREATED:20121126T173104Z
DESCRIPTION:Probing the Dark Sector with Euclid\nThe past decade has seen t
he emergence of the so-called "concordance model" of cosmology. In this mo
del\, the Universe started about 13.7 billion years ago in a Big Bang and
is now dominated by dark matter and dark energy. Together this poorly unde
rstood "dark sector" makes up about 95% of the Universe\, but the nature o
f these phenomena remains elusive. Weak gravitational lensing\, whereby th
e observed shapes of background galaxies are slightly distorted by foregro
und dark matter has proven to be one of the most useful ways to measure da
rk matter and dark energy. I'll explain the basics of weak lensing and out
line some key weak lensing results. Finally\, I'll discuss The European Sp
ace Agency's Euclid mission. NASA has recently agreed to partner on this a
mbitious mission to measure the dark sector in the 2020s. \nSpeaker: Dr. J
ason Rhodes\, JPL Research Scientist \n\nThe von Kármán Auditorium at JP
L\n4800 Oak Grove Drive\nPasadena\, CA\n
DTEND;TZID="Pacific Standard Time":20130117T200000
DTSTAMP:20121126T173104Z
DTSTART;TZID="Pacific Standard Time":20130117T190000
LAST-MODIFIED:20121126T173104Z
LOCATION:The von Kármán Auditorium at JPL
PRIORITY:5
SEQUENCE:0
SUMMARY;LANGUAGE=en-us:The von Kármán Lecture Series: 2013
TRANSP:OPAQUE
UID:040000008200E00074C5B7101A82E00800000000A07C87EFB7CBCD01000000000000000
010000000FDA5D840BFCDFC48BBF9B6FAB0A61237
X-ALT-DESC;FMTTYPE=text/html:\n\n\n\n\n\n\n\n\nProbing the Dark Sector with Euclid
\n\
nThe past decade has seen the emergen
ce of the so-called "\;concordance model"\; of cosmology. In this
model\, the Universe started about 13.7 billion years ago in a Big Bang an
d is now dominated by dark matter and dark energy. Together this poorly un
derstood "\;dark sector"\; makes up about 95% of the Universe\, bu
t the nature of these phenomena remains elusive. Weak gravitational lensin
g\, whereby the observed shapes of background galaxies are slightly distor
ted by foreground dark matter has proven to be one of the most useful ways
to measure dark matter and dark energy. I'll explain the basics of weak l
ensing and outline some key weak lensing results. Finally\, I'll discuss T
he European Space Agency's Euclid mission. NASA has recently agreed to par
tner on this ambitious mission to measure the dark sector in the 2020s.
\n\nSpeaker: \;&n
bsp\; \; \; \; \; \; Dr. Jason Rhodes\, JPL Research S
cientis<
SPAN LANG="en-us">t \; \;&
nbsp\; \; \; \; \;
\n
\n\nThe von Kár
mán Auditorium at JPL
\n4800 Oak Grove Drive
\nPasadena\, CA
\n\n\n
X-MICROSOFT-CDO-BUSYSTATUS:BUSY
X-MICROSOFT-CDO-IMPORTANCE:1
X-MICROSOFT-DISALLOW-COUNTER:FALSE
X-MS-OLK-AUTOFILLLOCATION:FALSE
X-MS-OLK-CONFTYPE:0
BEGIN:VALARM
TRIGGER:-PT10M
ACTION:DISPLAY
DESCRIPTION:Reminder
END:VALARM
END:VEVENT
END:VCALENDAR