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:
02.430 (Mainz Institute for Theoretical Physics, Johannes Gutenberg University)
Mainz Institute for Theoretical Physics, Johannes Gutenberg University
Staudingerweg 9 / 2nd floor, 55128 Mainz
Dark matter (DM) searches have undergone dramatic developments in the last decade. We expect 2015 and the following years to deliver a harvest of copious, high precision data, which will enable us to thoroughly test the most promising extensions of the Standard Model of particle physics. Thus, it is timely to start addressing the following key questions:
(i) How do hydrodynamical simulations contribute to our understanding of the Milky Way? And reversely, how to design future simulations in view of the available astronomical data?
(ii) How to use the astronomical data soon to be available in constraining the DM distribution in the Milky Way?
(iii) What are the consequences of both simulations and astronomical observations for the phenomenology of dark matter searches?
The proposed scientific program aims at addressing these questions by bringing together the three communities involved in this effort, namely astronomers, simulators and astroparticle physicists, in a unique and fruitful environment.