Event calendar file
3-11 July 2007
Merida, Mexico
Mexico/General timezone
- icrc2007@icrc2007.unam.mx
Support
HE 3.4
Place
Location: Merida, Mexico
Room: Kabah (Holiday Inn)
Date:
5 Jul 12:05 - 13:30
Timetable | Contribution List
Displaying 7
contributions
out of
7
In 2005, the MAGIC telescope observed an unprecedented rapid flare from the AGN Mrk
501. A fast and strong variability was found in several adjacent energy bands above
100 GeV and was used to search for correlated flux variations at different energies.
The resulting constraints on different possible Quantum Gravity effects have been
investigated and will be presented.
Presented by A. BILAND
on
5/7/2007
at
17:17
Cherenkov emissions of magnetic charges moving through matter will exceed those of
electric charges by several orders of magnitude. The AMANDA neutrino telescope is
therefore capable of efficiently detecting relativistic magnetic monopoles that pass
through its sensitive volume. We present a new limit on the flux of relativistic
magnetic monopoles based on the analysis of one
year of data tak
... More
Presented by Henrike WISSING
on
5/7/2007
at
17:53
The Short GAmma Ray Front Air Cherenkov Experiment is designed to search for bursts
of gamma rays above 200 MeV lasting from 60 nanoseconds to longer than 20
microseconds. The custom-designed trigger and data-acquisition system of SGARFACE
piggy-backs on the existing Whipple 10m telescope. The experiment has operated for
more than 3 years during which time about 1.2 million events were recorde
... More
Presented by M SCHROEDTER
on
5/7/2007
at
18:17
CUORICINO is a cryogenic detector running in Gran Sasso National Laboratories, Italy
since 2003.
With its 40.7 kg of 130TeO2 mass, in the form of an array of 62 crystals it has
proved the feasibility of CUORE experiment, whose aim is to be sensitive to value of
the effective neutrino mass as low as few tens of meV.
It has moreover set the currently lower limit on the lifetime of 130Te for
n
... More
Presented by Dr. Elena GUARDINCERRI
on
5/7/2007
at
17:05
Laser Interferometer Gravitational Wave Observatory (LIGO) consists of
three detectors, located in Hanford, Washington and Livingston, Louisiana,
which are designed to search for gravitational waves from astrophysical
sources. In November 2005, LIGO started col
... More
Presented by Dr. Shantanu DESAI
on
5/7/2007
at
17:41
Supermassive particles like magnetic monopoles, Q-balls and nuclearites may
emit light at subrelativistic speeds through different suggested mechanisms.
One of them is nucleon decay catalysis by magnetic monopoles, where the
decay products would emit Cherenkov radiation along a monopole track. The
emitted secondary light from subrelativistic particles could make them visible to
the AMAND
... More
Presented by Mr. Arvid POHL
on
5/7/2007
at
18:05
The search for rare massive particles in the cosmic radiation remains one of the main aim of non-accelerator particle
astrophysics. Experiments at high altitude allow lower mass thresholds with respect to detectors at sea level or
underground. We present here the analysis of the full SLIM detector (400 m^2) after 4y exposure at the
Chacaltaya site (5300m a.s.l.). A part is devoted to the stu
... More
Presented by Dr. stefano CECCHINI
on
5/7/2007
at
17:29
