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In order to enable an iCal export link, your account needs to have a key created. This key enables other applications to access data from within Indico even when you are neither using nor logged into the Indico system yourself with the link provided. Once created, you can manage your key at any time by going to 'My Profile' and looking under the tab entitled 'HTTP API'. Further information about HTTP API keys can be found in the Indico documentation.
I have read and understood the above.
In conjunction with a having a key associated with your account, to have the possibility of exporting private event information necessitates the creation of a persistent key. This new key is also associated with your account and whilst it is active the data which can be obtained through using this key can be obtained by anyone in possession of the link provided. Due to this reason, it is extremely important that you keep links generated with this key private and for your use only. If you think someone else may have acquired access to a link using this key in the future, you must immediately remove it from 'My Profile' under the 'HTTP API' tab and generate a new key before regenerating iCalendar links.
I have read and understood the above.
Permanent link for public information only:
Permanent link for all public and protected information:
The central array of the ARGO detector at the YangBaJing Cosmic Ray Laboratory
(4300 m a.s.l., Tibet, P.R. China) has been put into operation for physics runs.
It is made of 130 identical sub-units of 12 RPCs each ('cluster') covering a
surface of about 5800 m**2 with 92% active area. Signals are picked-up by external
electrodes of small size, thus allowing the sampling of EAS with high space
... More
Presented by Dr. Daniele MARTELLO
on
9/7/2007
at
14:42
A instrument to image medium energy gamma-rays is being designed for the
future NASA Advanced Compton Telescope (ACT) mission. This instrument
consists of a gas microwell imaging detector with an active detection volume of
approximately 1.6 m x 1.6m x 0.5m which is surrounded by a segmented
calorimeter. The use of the gas imager allows for the detection and tracking of
the recoil elect
... More
The HAWC (High Altitude Water Cherenkov) observatory is a proposed experiment that
combines a very high altitude site with the developed and proven Milagro water
Cherenkov technology. HAWC is a 150m x 150m pond of water located above 4100 m over
see level with a large field of view and a duty cycle higher than 95%. It observes
the relativistic particles and secondary gamma rays in extensive ai
... More
Presented by Dr. Maria Magdalena GONZALEZ SANCHEZ
on
9/7/2007
at
14:30
Reliable polarization measurements of photons from Gamma Ray Bursts (GRB)
would make the understanding of the GRB phenomenon progress enormously.
POLAR is a concept for an instrument that would enable such a measurement.
We will report about the first results of the performance of a prototype
of this instrument and compare it with Monte-Carlo prediction.
Presented by Dr. Giovanni LAMANNA
on
9/7/2007
at
14:18
The CANGAROO-III telescope system for very-high-energy gamma-ray astrophysics
consists of four 10-m atmospheric Cherenkov telescopes located near Woomera, South
Australia.
We have been observing southern-sky objects since March 2004.
Here we report on the status of the system and some recent results from CANGAROO-III
observations.
The 17m diameter MAGIC telescope is currently the largest single dish
Cherenkov telescope for gamma ray astronomy. Within the year 2007 it
will be upgraded with a second telescope MAGIC-II.
Stereo observations will improve the sensitivity of the observatory by a
factor of 2 and help to lower the energy threshold.
The design, status and expected performance of MAGIC-II will be presented.
Presented by Dr. Florian GOEBEL
on
9/7/2007
at
13:42
VERITAS is an atmospheric Cherenkov telescope array designed
to study astrophysical sources of very high energy gamma radiation.
Located in southern Arizona, USA, the array consists of four
12-m diameter imaging Cherenkov telescopes. All four telescopes
have been deployed at the basecamp of the Whipple Observatory
and they became fully operational in early 2007. This paper
describes the
... More
Presented by Dr. Gernot MAIER
on
9/7/2007
at
13:30
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