In order to enable an iCal export link, your account needs to have an API 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.
Additionally to having an API key associated with your account, exporting private event information requires the usage of a persistent signature. This enables API URLs which do not expire after a few minutes so while the setting is active, anyone in possession of the link provided can access the information. Due to this, it is extremely important that you keep these links 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 create a new key pair on the 'My Profile' page under the 'HTTP API' and update the iCalendar links afterwards.
Permanent link for public information only:
Permanent link for all public and protected information:
(Universität Erlangen & DESY Zeuthen)
Main Lecture Hall (GSI)
Main Lecture Hall
The particles with the highest known energies in the universe are cosmic rays. Energies unreachable by human accelerators. But even after more than 100 years since their discovery, it is still unknown which astronomical objects can create such ultra-high energetic charged particles. Detecting ultra-high energy neutrinos may resolve the problem. Neutrinos travel unimpeded in straight lines, thereby revealing their sources, which they share with cosmic rays. The optical detectors, most notably IceCube at the South Pole, have started the exciting field of neutrino astronomy. However, even these enormous detectors do not monitor enough ice to be able to detect the increasingly smaller flux of neutrinos of the highest energies. I will elaborate why radio detectors provide enough sensitivity, what technological challenges we meet on the way and how the neutrino community will build a large detector to discover cosmogenic neutrinos and move to standard operation mode in neutrino astronomy.