We are delighted to announce this fantastic public & alumni event hosted by our department together with the team at IceCube South Pole neutrino Observatory (US & South Pole).

Our Head of Particle Physics Professor Daniela Bortoletto will be hosting a live link-up with Josh Veitch-Michaelis and Martin Wolf, IceCube winterovers who will be talking to us live from Antarctica. Professor Jim Madsen, Executive Director Wisconsin IceCube Particle Astrophysics Center and Gwenhaël de Wasseige, MSCA Individual Fellow, Laboratoire Astroparticule et Cosmologie will also be joining us to share their work and talk all things neutrino.

You may have heard these news lately, about IceCube, and this is the perfect time to join us, learn what happens there and how the research is done, and ask all the questions you may have.

Please see the following links for more information about the IceCube Neutrino Observatory and our speakers:

• IceCube South Pole Neutrino Observatory
• Professor Jim Madsen
• Gwenhaël de Wasseige
• Life at the Pole
• Instagram @icecube_neutrino

For questions about this event, please contact alumni@physics.ox.ac.uk.

We look forward to seeing you on 11th June! EVERYONE is welcome to join us!

The link to join will be sent to all registrants a couple of days before the event, and again on the day of the event around 1pm UK time, for late registrations. To help us manage better, please register if you can attend.

Registration closes at 12 noon on the day of the event.

Please note:

• We will be connected via live video link to the South Pole where the Observatory is located. While we will do all we can to ensure the connection is stable, it may be that suboptimal weather conditions prevent this part of the event from going ahead.
• Winterovers will be indoors as it will be before dawn in Antarctica.
• If you are a member of the Henry Moseley Circle, you would have already received an invitation and link to register, please use that one.

All images Copyright IceCube. Please seek authorisation before sharing.