BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//INPA - ECPv6.8.3//NONSGML v1.0//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
X-ORIGINAL-URL:https://inpa.lbl.gov
X-WR-CALDESC:Events for INPA
REFRESH-INTERVAL;VALUE=DURATION:PT1H
X-Robots-Tag:noindex
X-PUBLISHED-TTL:PT1H
BEGIN:VTIMEZONE
TZID:America/Los_Angeles
BEGIN:DAYLIGHT
TZOFFSETFROM:-0800
TZOFFSETTO:-0700
TZNAME:PDT
DTSTART:20220313T100000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:-0700
TZOFFSETTO:-0800
TZNAME:PST
DTSTART:20221106T090000
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=America/Los_Angeles:20221104T120000
DTEND;TZID=America/Los_Angeles:20221104T130000
DTSTAMP:20260427T214245
CREATED:20221031T211901Z
LAST-MODIFIED:20221031T211947Z
UID:1278-1667563200-1667566800@inpa.lbl.gov
SUMMARY:Speaker: Dan Werthimer (UC Berkeley (SETI) "What's New in SETI and High Performance Signal Processing\,  and The PANOSETI IR/Visible Ultra-Wide Field Nanosecond Time Scale Transient Search"
DESCRIPTION:Abstract: \nDan will review current and SETI radio and optical searches\, and also review CASPER open source technologies for real time signal processing instrumentation. The CASPER collaboration develops open source hardware\, software\, GPUware\, FPGA gateware\, tools\, libraries\, reference designs\, tutorials\, training videos\, and workshops for astronomy instrumentation.\nCASPER instrumentation is utilized mostly for radio astronomy\, but also for physics\, medicine\, genomics\, and engineering. More info at http://casper.berkeley.edu \nThe PANOSETI experiment searches a largely unexplored parameter space\, observing a large field of view simultaneously (4\,450 degrees) for nanosecond to second time scale transients at visible and near-IR wavelengths. The PANOSETI observatory employs two domes separated by ~1 km. Data from the two domes is cross-correlated to distinguish between astrophysical events and atmospheric phenomena (eg: Cherenkov radiation). Each PANOSETI dome contains ~45 telescopes; each telescope covers a 10 by 10 degree field. We have deployed a prototype PANOSETI observatory at Lick Observatory; where we also plan to build a full scale system. The small aperture\, wide field-of-view\, and low cost of the PANOSETI telescopes make them well-suited for high energy gamma-ray astronomy.
URL:https://inpa.lbl.gov/event/speaker-dan-werthimer-uc-berkeley-seti-whats-new-in-seti-and-high-performance-signal-processing-and-the-panoseti-ir-visible-ultra-wide-field-nanosecond-time-scale-transient-search/
LOCATION:50A-5132 / https://lbnl.zoom.us/j/95016696011?pwd=Tk1XOW1Xd3RYRnlsc2tEYmRWZlVVZz09\, One Cyclotron Road\, 50A-5132\, Berkeley\, CA\, 94720\, United States
ORGANIZER;CN="Kevin Wood":MAILTO:KWood@lbl.gov
END:VEVENT
END:VCALENDAR