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:
Imprints of dark matter physics in cosmological large-scale structure
The properties of neutrinos and dark matter candidates produce characteristic imprints in the large-scale distribution of matter in the Universe. This has previously been used to place constraints on, e.g., the total mass of neutrinos. The next generation of astronomical galaxy surveys, e.g. from the Uppsala-affiliated projects 4MOST and the Square Kilometre Array, promise to vastly increase precision, covered area, and observational depth. This will enable novel, stringent constraints to be placed on the masses of neutrinos and dark matter candidates. As a specific case, I describe how the novel probe of cosmic voids can break awkward parameter degeneracies to produce robust constraints. I outline the first cosmological constraints derived from void abundance, and discuss the potential of void and galaxy cluster abundances to constrain the mass of neutrinos and reject an inverted neutrino mass hierarchy.
Based on ApjL 820(1), 7 (2016); PRD 97(10), 103504 (2018); PRD 99(6), 063525 (2019), arXiv:1810.02680, arXiv:1811.02743, arXiv:1903.05161