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:
(Canadian Institute for Theoretical Astrophysics, Toronto (CA))
Aula Rasetti (Dipartimento di Fisica - ED. G.Marconi)
Dipartimento di Fisica - ED. G.Marconi
Planck, ACT, and SPT are mapping out the microwave sky in unprecedented detail. At the same time, future surveys with such facilities as CHIME, LSST, and SKA will revolutionize the amount of information available to us about the formation of the first stars and black holes, galaxies, and the large scale structure of the universe. Making sense of all this data will require cosmological simulations accurate over a much larger dynamic range than currently possible. I will describe the current open questions that can be answered with this data and present the new computational techniques we are developing to tackle this problem. Particular focus will be placed upon fast reionization simulations that use the excursion set formalism and accurate large scale structure calculations using a massively parallel implementation of the peak patch approach.