BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//Erlangen Centre for Astroparticle Physics - ECPv6.2.3.2//NONSGML v1.0//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
X-WR-CALNAME:Erlangen Centre for Astroparticle Physics
X-ORIGINAL-URL:https://ecap.nat.fau.de
X-WR-CALDESC:Events for Erlangen Centre for Astroparticle Physics
REFRESH-INTERVAL;VALUE=DURATION:PT1H
X-Robots-Tag:noindex
X-PUBLISHED-TTL:PT1H
BEGIN:VTIMEZONE
TZID:Europe/Berlin
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20170326T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20171029T010000
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=Europe/Berlin:20170706T090000
DTEND;TZID=Europe/Berlin:20170706T100000
DTSTAMP:20260426T211426
CREATED:20170705T110024Z
LAST-MODIFIED:20170705T110024Z
UID:822-1499331600-1499335200@ecap.nat.fau.de
SUMMARY:Francois Brun - The H.E.S.S. Galactic Plane Survey
DESCRIPTION:H.E.S.S. (High Energy Stereoscopic System) is a hybrid array of five Imaging Atmospheric Cherenkov Telescopes observing the very high energy gamma-ray sky. In the past decade\, this experiment has significantly contributed to the field of ground-based gamma-ray astronomy. In particular\, the H.E.S.S. Galactic plane survey (HGPS)\, conducted from 2004 to 2013\, was the first high-resolution (~0.1 deg) and sensitive (~1.5% Crab Nebula point-source sensitivity) survey of the Milky Way in TeV gamma-rays. Comprising ~2800-hrs of observation time\, it revealed the existence of a diverse population of cosmic accelerators in the Galaxy. In this talk I will present an overview of the results from this decade-long H.E.S.S. survey program.
URL:https://ecap.nat.fau.de/index.php/event/seminar-2017-07-05-francois-brun/
LOCATION:ECAP\, room 307\, Erwin-Rommel-Str 1\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
END:VEVENT
END:VCALENDAR