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:
Polar Particle Physics: Measuring Fundamental Neutrino Properties with Antarctic Neutrino Detectors
(Radboud University Nijmegen)
WAT112 (Watanabe Hall)
Large-scale Cherenkov neutrino detectors, such as the IceCube Neutrino Observatory at the geographic South Pole, are at the forefront of the search for astrophysical neutrino sources in the TeV energy range. Additionally, these detectors are excellent instruments with which to explore fundamental neutrino properties and to search for physics beyond the Standard Model. I will discuss several of these possibilities, including searches for violation of Lorentz invariance and sterile neutrinos, using the atmospheric muon neutrino flux as a "test beam". Low-energy extensions of IceCube may also enable determination of the neutrino mass heirarchy, while novel neutrino detectors such as the Askaryan Radio Array (ARA) will extend the search to higher energies and cosmological baselines using cosmogenic neutrinos.