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:
Magnetic Fields in Early Stellar Evolution: The Case of Upper Scorpius
Absolute ages estimated for identifiably young stellar populations strongly depend on which stars are used in the age dating analysis. Cooler K- and M-type stars typically yield ages that are systematically younger by a factor of two compared to warmer A-, F-, and G-type stars. In this talk, I will highlight efforts to understand these age discrepancies as the result of magnetic inhibition of convection in cool young stars. Specifically, I will focus on the adoption of magnetic stellar evolution models to derive a consistent 10 Myr age for the Upper Scorpius subgroup of the Scorpius-Centaurus OB Association. Multiple pieces of evidence in support of this explanation will be presented along with several remaining problems and uncertainties.