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:
The low side of the dark side - Prof. Jochen Schieck (Österreichische Akademie der Wissenschaften and Technische Universität Wien)
Main Auditorium (MPP)
Max-Planck-Institut für Physik
Föhringer Ring 6
The quest for the particle nature of Dark Matter is one of the big open questions of modern physics. A well motivated candidate for Dark Matter is the so-called WIMP - a weakly interactive massive particle. Recently several theoretically well-motivated models with Dark Matter candidates in a mass region below the WIMP mass-scale gained also a lot of interest, theoretically and experimentally. The CRESST II experiment located at the Gran Sasso laboratory in Italy is optimised for the detection of the elastic scattering of these low mass Dark Matter particles with nuclei. Besides the search for Dark Matter particles scattering with nuclei, we present a new search for so-called Dark Photons, also based on CRESST data. Finally the potential and the layout of a future silicon based dark matter experiment, dedicated to sub-GeV Dark Matter detection, is discussed.