Speaker
Qi Feng
(SAO)
Description
In the last decade, IceCube has enabled multi-messenger astronomy with neutrinos and revolutionized the field of astroparticle physics. By combining gamma-ray and neutrino data, significant progress has been made in understanding the most energetic phenomena in the universe. However, there is still much to be explored and understood. As the next-generation instruments for both messengers, such as the Cherenkov Telescope Array (CTA) and IceCube-Gen2, are on the horizon, it is crucial to consider the prospects and strategies for multi-messenger science. The upcoming era of IceCube-CTA synergy holds great potential for advancing our understanding of the universe.
| Do you describe your self as early career? | yes |
|---|---|
| Please add details of experiment/project that this abstract corresponds to? | The CTA SCT Project |
| Please select if remarks will be in person or on zoom | On zoom |
Primary authors
Qi Feng
(SAO)
The CTA SCT Project