BEGIN:VCALENDAR
VERSION:2.0
X-WR-CALNAME:Zwicky Conference
PRODID:-//Apple Computer\, Inc//iCal 2.0//EN
X-WR-RELCALID:B4C43404-7D25-4BA6-B77A-3FA0B5214801
X-WR-TIMEZONE:US/Pacific
CALSCALE:GREGORIAN
METHOD:PUBLISH
BEGIN:VTIMEZONE
TZID:US/Pacific
LAST-MODIFIED:20050524T035825Z
BEGIN:DAYLIGHT
DTSTART:20050403T100000
TZOFFSETTO:-0700
TZOFFSETFROM:+0000
TZNAME:PDT
END:DAYLIGHT
BEGIN:STANDARD
DTSTART:20051030T020000
TZOFFSETTO:-0800
TZOFFSETFROM:-0700
TZNAME:PST
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T101000
DTEND;TZID=US/Pacific:20050525T102500
SUMMARY:Derek Fox
UID:2A26E103-5EC6-4ABD-A6A7-62F5EA04C4AB
SEQUENCE:7
DTSTAMP:20050524T031418Z
DESCRIPTION:GRB effort at P60\, potentially including SN science or mult
 i-telescope work (Quest -> P60)
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T090000
DTEND;TZID=US/Pacific:20050525T093000
SUMMARY:Coffee
UID:91B9EFDE-C562-4269-B660-10E6067234E6
SEQUENCE:9
DTSTAMP:20050524T030900Z
DESCRIPTION:Meet at the SSL conference room
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T143000
DTEND;TZID=US/Pacific:20050525T144500
SUMMARY:Greg Taylor
UID:67F18FB9-B921-4AE4-AE80-703DF38E5602
SEQUENCE:6
DTSTAMP:20050524T034253Z
DESCRIPTION:Exploring the Transient Universe with the Long Wavelength Ar
 ray\n\nThe Long Wavelength Array (LWA) would provide mJy sensitivity at\
 narcsecond level resolution in the relatively unexplored frequency\nrang
 e 20-80 MHz.  With a field of view of 3 degrees (at 70 MHz) and\nmillise
 cond time resolution this instrument will be uniquely\nwell suited to th
 e discovery of transient events.  Giant Flares from\nmagnetars\, like th
 e recent outburst from SGR1806-20 would be\ndetectable in our Galaxy and
  as far away as M31.  Enigmatic\nobjects like the recently discovered Ga
 lactic Center Radio Transient\nJ1745-2009 could be closely monitored\, a
 nd similar sources readily\ndiscovered.  In addition to pointed studies\
 , the LWA Demonstrator\nstation currently under construction has the cap
 ability to do all-sky\ntransient monitoring.  This could detect coherent
  emission from\nhigh-energy cosmic ray air-showers\, prompt emission ass
 ociated with\nGRBs\, extra-solar planets\, or new phenomena.\n
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T154000
DTEND;TZID=US/Pacific:20050525T155500
SUMMARY:Dan Wertheimer
UID:7C78BDF8-9EE4-41F7-8F4A-F631EE9070D5
SEQUENCE:7
DTSTAMP:20050524T034640Z
DESCRIPTION:Evaporating Black Holes
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T161000
DTEND;TZID=US/Pacific:20050525T162500
SUMMARY:Brad Hansen
UID:A5DE9877-13C0-4622-98C4-73A1B195AFBF
SEQUENCE:7
DTSTAMP:20050524T034854Z
DESCRIPTION:As Yet Unobserved Transient Phenomena
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T102500
DTEND;TZID=US/Pacific:20050525T104000
SUMMARY:Tom Vestrand
UID:77B7FF1C-17B9-4ED7-958A-01CADC04489C
SEQUENCE:8
DTSTAMP:20050524T031512Z
DESCRIPTION:Thinking Telescopes\, RAPTOR\, and GRB Follow-up
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T094000
DTEND;TZID=US/Pacific:20050525T095500
SUMMARY:Don Backer
UID:FED44D42-B88D-421E-9D94-0115C7B16579
SEQUENCE:6
DTSTAMP:20050524T030954Z
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T114500
DTEND;TZID=US/Pacific:20050525T120000
SUMMARY:Alicia Soderberg
UID:7631A586-4F10-4A0A-97E7-FDCF610B0522
SEQUENCE:5
DTSTAMP:20050524T031808Z
DESCRIPTION:Radio Observations of SNe Ibc
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T141500
DTEND;TZID=US/Pacific:20050525T143000
SUMMARY:Don Backer
UID:1CDBCB6F-0925-46DF-87F1-BE5FA55A0F70
SEQUENCE:5
DTSTAMP:20050524T034148Z
DESCRIPTION:PAPER: Portable Array to Prove Epoch of Reionization
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T144500
DTEND;TZID=US/Pacific:20050525T150000
SUMMARY:Paul Price
UID:6E6AE434-1030-4C8A-93C3-3E6243509580
SEQUENCE:5
DTSTAMP:20050524T034423Z
DESCRIPTION:PanStarrs
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T123000
DTEND;TZID=US/Pacific:20050525T134500
SUMMARY:Lunch
UID:F05CD9A4-DDAE-439C-8E3C-573A7362B6B7
SEQUENCE:3
DTSTAMP:20050524T033840Z
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T121500
DTEND;TZID=US/Pacific:20050525T123000
SUMMARY:Edo Berger
UID:84E24787-9FB8-474A-96E1-2DF0F9FD2653
SEQUENCE:6
DTSTAMP:20050524T033815Z
DESCRIPTION:Brown Dwarf
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T111500
DTEND;TZID=US/Pacific:20050525T113000
SUMMARY:George Djorgovski
UID:A10E04C8-FBD0-4C20-ACAD-B5797D657367
SEQUENCE:6
DTSTAMP:20050524T031634Z
DESCRIPTION:Exploring the time domain\, and the PQ survey update
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T134500
DTEND;TZID=US/Pacific:20050525T140000
SUMMARY:Douglas Bock
UID:E5401134-C217-41D4-9771-AAC0564355FF
SEQUENCE:5
DTSTAMP:20050524T033947Z
DESCRIPTION:Transient Detection with CARMA
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T120000
DTEND;TZID=US/Pacific:20050525T121500
SUMMARY:Michael Muno
UID:C0D99C1D-F189-4039-B29A-F5CFF5BA1E3B
SEQUENCE:6
DTSTAMP:20050524T031857Z
DESCRIPTION:What are the Fast X-ray Transients Near the Galactic Center?
 
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T140000
DTEND;TZID=US/Pacific:20050525T141500
SUMMARY:Geoff Bower
UID:49284E8B-C970-4752-A06B-295B8866C9C6
SEQUENCE:6
DTSTAMP:20050524T034119Z
DESCRIPTION:Transients with the ATA
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T155500
DTEND;TZID=US/Pacific:20050525T161000
SUMMARY:Elliot Bloom
UID:F457316B-8947-4385-A864-A4E9FE1A6F87
SEQUENCE:12
DTSTAMP:20050524T034819Z
DESCRIPTION:Overview of the GLAST mission GRB capabilities
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T164000
DTEND;TZID=US/Pacific:20050525T170000
SUMMARY:Brian Schmidt
UID:690DA191-A0EF-4F88-82BD-ABE30AD12321
SEQUENCE:9
DTSTAMP:20050524T035218Z
DESCRIPTION:Transient Sources\, The Southern Sky Survey and the SkyMappe
 r Telescope\n\nMt Stromlo Observatory is replacing the Great Melbourne T
 elescope\,\ndestroyed in bushfires on the 18th of January\, 2003\, with 
 the\nSkyMapper Telescope - with an 8sq-degree field of view. This telesc
 ope\nwith be equipped with a 268 Million Pixel Camera made up of 32 E2V\
 n40micron deep depleted CCDs\, providing 5 square degrees of sky\ncovera
 ge with 0.5 arcsecond pixels and a 20 second readout time. The\ninstrume
 nt has reasonable throughput from the 320nm-1micron\, and will\nbe dedic
 ated 75% to the Southern Sky Survey\, a survey covering the\nentirety of
  the southern celestial hemisphere in 6 filters (6 epochs\neach) includi
 ng g\,r\,i\,z\, along with a stromgren u\, and a DDO-38\nfilter. These l
 atter two filters will provide gravity and metallicity\ninformation for 
 more than 100\,000\,000 stars in the survey. Total depth\nof the survey 
 will be approximately 0.5-1mag deeper than the SDSS\nsurvey\, with indiv
 idual epochs approx 0.5 mags less sensitive than the\nSDSS survey. Surve
 y is planned to commence at the end of 2006 and\nfinish in 2009. Data wi
 ll be made available to the public in as short\nof time as possible.
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T150000
DTEND;TZID=US/Pacific:20050525T151500
SUMMARY:Kem Cook
UID:C8EA272B-989B-49EA-A8C0-68065BA0CCC7
SEQUENCE:5
DTSTAMP:20050524T034528Z
DESCRIPTION:LSST: A Tidal Wave of Transients
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T104000
DTEND;TZID=US/Pacific:20050525T111500
SUMMARY:Coffee Break
UID:A54F7B86-F4CD-4BF3-A1A9-6C10F9365705
SEQUENCE:6
DTSTAMP:20050524T031557Z
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T095500
DTEND;TZID=US/Pacific:20050525T101000
SUMMARY:Weidong Li
UID:7E69DA3E-B113-4B05-8B19-AEB7B76F0258
SEQUENCE:9
DTSTAMP:20050524T031322Z
DESCRIPTION:KAIT and its SN/GRB
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T170000
DTEND;TZID=US/Pacific:20050525T171500
SUMMARY:John Vallerga
UID:C0051A86-14E2-4921-A180-F919A21F3015
SEQUENCE:7
DTSTAMP:20050524T035334Z
DESCRIPTION:Photon counting detectors for the visible region\n\nWe prese
 nt details of the NSF-funded research program to develop high-time resol
 ution photon counting  detectors for visible wavelength astronomy being 
 carried out by  the Experimental Astrophysics Group at the Space Science
 s Laboratory at UC Berkeley. We will discuss the Medipix image-tube dete
 ctor\, currently being developed for adaptive optics applications and a 
 sub-millisecond sealed tube photon counter based on GaAs to be used for 
 polarization studies of individual pulsar pulses. Finally we show empiri
 cal data from the GALEX mission that outlines the utility of high time r
 esolution detectors for recording dMe flares and  for tracking space deb
 ris.
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T171500
DTEND;TZID=US/Pacific:20050525T173000
SUMMARY:Shri Kulkarni
UID:6D1FD5DD-0404-45B7-86B6-34989F07946C
SEQUENCE:6
DTSTAMP:20050524T035402Z
DESCRIPTION:Closing Remarks: A Look Ahead
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T173000
DTEND;TZID=US/Pacific:20050525T180000
SUMMARY:Closing Reception
UID:FFDA0839-4B44-4BE7-B269-3202E9EC07FE
SEQUENCE:4
DTSTAMP:20050524T035426Z
END:VEVENT
BEGIN:VEVENT
LOCATION:SSL Conference Room
DTSTAMP:20050524T035709Z
UID:2C2CF8E0-D05C-4E75-BEB5-036670031ED0
SEQUENCE:8
URL;VALUE=URI:http://astro.berkeley.edu/~jbloom/zwicky.html
DTSTART;TZID=US/Pacific:20050525T084500
SUMMARY:Zwicky Conference
DTEND;TZID=US/Pacific:20050525T180000
DESCRIPTION:Call 510-229-8163 with last minute questions or jbloom@astro
 .berkeley.edu
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T162500
DTEND;TZID=US/Pacific:20050525T164000
SUMMARY:Roy Williams
UID:E1B3258C-3A8A-440C-BCC2-22935DBFC9B5
SEQUENCE:8
DTSTAMP:20050524T035105Z
DESCRIPTION:VOEvents: Connecting the EM spectrum (and others)
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T093000
DTEND;TZID=US/Pacific:20050525T094000
SUMMARY:Leo Blitz
UID:BC1ED757-351F-48F4-B3FF-59076DBAEE33
SEQUENCE:10
DTSTAMP:20050524T030916Z
DESCRIPTION:Welcome
END:VEVENT
BEGIN:VEVENT
DTSTAMP:20050524T034609Z
UID:5DEEDD8C-AA0E-4686-A8F8-E08957A94429
SEQUENCE:7
URL;VALUE=URI:http://hello.com
DTSTART;TZID=US/Pacific:20050525T151500
SUMMARY:Coffee!
DTEND;TZID=US/Pacific:20050525T154000
DESCRIPTION:number 2
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=US/Pacific:20050525T113000
DTEND;TZID=US/Pacific:20050525T114500
SUMMARY:Avishay Gal-Yam
UID:4B440F26-F61D-4973-8E43-133FC59E12D9
SEQUENCE:6
DTSTAMP:20050524T031730Z
DESCRIPTION:A complete characterization of the transient radio sky down 
 to 6 mJy at 1.4 GHz
END:VEVENT
END:VCALENDAR