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:
Greg Ashton (Monash University) will present "Maximising the science of gravitational-wave observatories"
The era of gravitation-wave astronomy is well underway. The third LIGO-Virgo observing run recently concluded bringing the total of detections and candidates to 67 and future observing runs with improved detectors will continue to advance the number and variety of signals we observe. These signals and their multi-messenger counterparts encode information which can answer some of the big questions facing science today. In this talk, I will describe how a Bayesian inference framework ensures we maximise the science of gravitational-wave observatories. From gold-plating marginal candidates to quantifying the astrophysical probability of a signal and inferring the source properties using the most sophisticated waveform models. I'll describe many of the challenges and limiting factors we currently face such the handling of systematic uncertainty in our physical signal models and our models of the noise. I'll then conclude by discussing how this framework can enable multi-messenger inference and the impacts it is already having across astrophysics.