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:
Accreting black hole binaries have been in focus of the X-ray
telescopes for the last half a century. Yet, radiative mechanisms leading
to a formation of the high energy photons along with the accretion flow
geometry in these objects are still being debated. Recent discovery of
complex interconnection of the optical and X-ray light-curves opened a new
path to explore physical processes operating in these objects. A number of
observables such as high optical luminosity, rapid variability and presence
of quasi-periodic oscillations at these wavelengths as well as complex
optical/X-ray cross-correlation cannot be explained in terms of the
standard accretion disc model. I will describe how the whole set of these
properties can be explained in terms of the hot accretion flow model.