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METHOD:PUBLISH
X-WR-CALNAME:INPA
X-ORIGINAL-URL:https://inpa.lbl.gov
X-WR-CALDESC:Events for INPA
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BEGIN:VTIMEZONE
TZID:America/Los_Angeles
BEGIN:DAYLIGHT
TZOFFSETFROM:-0800
TZOFFSETTO:-0700
TZNAME:PDT
DTSTART:20190310T100000
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TZOFFSETFROM:-0700
TZOFFSETTO:-0800
TZNAME:PST
DTSTART:20191103T090000
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BEGIN:VEVENT
DTSTART;TZID=America/Los_Angeles:20190104T120000
DTEND;TZID=America/Los_Angeles:20190104T130000
DTSTAMP:20260526T133100
CREATED:20181017T180240Z
LAST-MODIFIED:20181017T180240Z
UID:463-1546603200-1546606800@inpa.lbl.gov
SUMMARY:Holiday
DESCRIPTION:
URL:https://inpa.lbl.gov/event/holiday-3/
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Los_Angeles:20190104T120000
DTEND;TZID=America/Los_Angeles:20190104T130000
DTSTAMP:20260526T133100
CREATED:20181207T193104Z
LAST-MODIFIED:20181207T193104Z
UID:486-1546603200-1546606800@inpa.lbl.gov
SUMMARY:Matt Shaw (JPL) - Silicon nanowire single photon detectors
DESCRIPTION:TBA
URL:https://inpa.lbl.gov/event/matt-shaw-jpl-silicon-nanowire-single-photon-detectors/
LOCATION:INPA Common Room\, 50-5026
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Los_Angeles:20190111T120000
DTEND;TZID=America/Los_Angeles:20190111T130000
DTSTAMP:20260526T133100
CREATED:20181003T214303Z
LAST-MODIFIED:20181003T214303Z
UID:446-1547208000-1547211600@inpa.lbl.gov
SUMMARY:Aleksandar Cikota (LBNL)
DESCRIPTION:TBA
URL:https://inpa.lbl.gov/event/aleksandar-cikota-lbnl/
LOCATION:50A-5132- Sessler\, 50A-5132 Sessler Conference Room\, CA
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Los_Angeles:20190118T120000
DTEND;TZID=America/Los_Angeles:20190118T130000
DTSTAMP:20260526T133100
CREATED:20181003T214412Z
LAST-MODIFIED:20190116T211131Z
UID:448-1547812800-1547816400@inpa.lbl.gov
SUMMARY:Silvia Scorza (Snolab\, Sudbury) - Updates from SNOLAB
DESCRIPTION:Astroparticle physics experiments searching for rare events\, such as neutrinoless double beta decay and dark matter particles interactions\, have to be shielded from background radiation that would interact and hide the physics of interest\, and have to exhibit a radioactive background as low as possible. Therefore\, underground site are preferred. Being protected from cosmic rays\, the underground environment provides the conditions necessary for experiments dealing with such rare or exotic interactions. \nSNOLAB is one such facility\, based at a depth of 2km in the Vale Creighton mine near Sudbury\, Ontario. The lab hosts a number of neutrino and dark matter experiments as well as new biology and genomic experiments making use of the unique facility.
URL:https://inpa.lbl.gov/event/silvia-scorza-snolab-sudbury/
LOCATION:50A-5132- Sessler\, 50A-5132 Sessler Conference Room\, CA
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Los_Angeles:20190125T120000
DTEND;TZID=America/Los_Angeles:20190125T130000
DTSTAMP:20260526T133100
CREATED:20181003T214506Z
LAST-MODIFIED:20190417T151057Z
UID:450-1548417600-1548421200@inpa.lbl.gov
SUMMARY:NO INPA SEMINAR MTG
DESCRIPTION:
URL:https://inpa.lbl.gov/event/anna-ijjas-harvard-cfa/
LOCATION:50A-5132- Sessler\, 50A-5132 Sessler Conference Room\, CA
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=America/Los_Angeles:20190130T120000
DTEND;TZID=America/Los_Angeles:20190130T130000
DTSTAMP:20260526T133100
CREATED:20190118T190235Z
LAST-MODIFIED:20190130T174941Z
UID:496-1548849600-1548853200@inpa.lbl.gov
SUMMARY:SPECIAL - Brittany Kamai (CalTech) - Looking further back with LIGO
DESCRIPTION:Gravitational wave detectors require constant innovation in detector technology to meet the growing needs of the astrophysics community. With improved sensitivity\, we can move beyond the measurements in the local universe and perform precision tests of cosmology. I will discuss our efforts to reduce the amount of low frequency noise within the LIGO detectors\, which has a direct impact on our ability to measure heavier mass black hole mergers further out into the universe. I will focus on a proposed major upgrade to the LIGO detectors that will use silicon optics cooled to cryogenic temperatures. Additionally\, I will discuss ideas for a passive seismic isolation system that uses advances in seismic cloaking technology. These improvements will extend distance measurements on gravitational wave mergers from the local universe out to much higher redshifts.
URL:https://inpa.lbl.gov/event/special-brittany-kamai-caltech/
LOCATION:INPA Common Room\, 50-5026
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END:VCALENDAR