| Date | Activity | Name | Title | Video Available | Slides Available |
| 2024-11-05 | colloq | | Muon Colliders: the Next Generation of Particle Accelerators | Yes | No |
| 2024-08-28 | firstbillion_c24 | | Metal-poor massive stars in the first galaxies and next-door (H) | Yes | No |
| 2024-08-27 | firstbillion_c24 | | Lightning talk: The Next Generation Deep Extragalactic Exploratory Public (NGDEEP) Survey | Yes | No |
| 2023-05-15 | nanoassembly_c23 | | Next steps in patchy particle assembly engineering | Yes | No |
| 2023-03-17 | holonomy_s23 | | Enumerative invariants: what we did, and where to go next | Yes | Yes |
| 2023-02-16 | cosmicweb23 | | DARWIN: Dazzling Realization of dWarf galaxies In the Next generation of cosmological hydrodynamic simulations | Yes | Yes |
| 2022-04-20 | gwaves_c22 | | Numerical relativity for next-generation gravitational-wave observatories | Yes | Yes |
| 2021-11-24 | transtar21 | | Next-Generation Simulations of the Remarkable Deaths of Massive Stars | Yes | Yes |
| 2021-01-27 | nsbp_iss | | Next-Generation Simulations of The Remarkable Deaths of Massive Stars | Yes | Yes |
| 2019-06-25 | gravast_c19 | | Black Holes: the Next Generation | Yes | No |
| 2019-05-20 | exostar_c19 | | The Next Frontiers for Asteroseismology | Yes | No |
| 2019-05-15 | friends | | The Climates of Other Worlds: Searching for the Next Habitable Planet | Yes | Yes |
| 2018-01-25 | suspensions_c18 | | Quantitative Light Microscopy of Dense Suspensions: Colloid Science at the Next Decimal Place | Yes | Yes |
| 2017-08-22 | intertwined17 | | How to find the next unconventional high temperature superconductors | Yes | Yes |
| 2016-06-09 | colduniv16 | | From 0 to 100 in 5 years: how we will solve reionization before your next student graduates. | Yes | Yes |
| 2016-05-24 | lhc_c16 | | Next-to-soft radiative corrections in QCD | Yes | Yes |
| 2016-05-02 | experlhc16 | | Discussion: Status of naturalness and next steps to exclude natural SUSY spectra. | Yes | No |
| 2016-04-07 | lhc16 | | Discussion: Next-to-next-to-leading order approximation to perturbative QCD at the LHC[Podcast][Aud][Cam] Session run by ExperLHC16 | Yes | Yes |
| 2014-11-04 | neutrinos_c14 | | Reactor Neutrinos: Recent Results and Next Steps | Yes | Yes |
| 2013-07-08 | lhc_c13 | | Precision Higgs physics: the next step | Yes | Yes |
| 2011-11-04 | asteroseismo11 | | The DA White Dwarf Pulsator (ZZ Ceti) HS 0507+0434B: The Main Target of the Next WET Campaign | Yes | No |
| 2010-02-26 | evocell10 | All ParticipantsRelated Words: 1, 2, 20, 4, bloc, breakout, bring, closing, discussion, room, summary | Discussion: What To Do Next? | Yes | No |
| 2008-12-15 | qspinhall_m08 | | Discussion: Next Generation Experiments | Yes | Yes |
| 2008-11-21 | fluctuate08 | | "van der Waals" "Hamaker" "Casimer" "Lifshitz" "fluctuation" "electrodynamic": Where Now? What Next? | Yes | Yes |
| 2007-10-19 | stars07 | | Simulations of Population III Star Formation: What's Next? | Yes | Yes |
| 2006-08-10 | atto06 | | Attosecond Pump-Probe Experiments at Next Generation Light Sources | Yes | No |
| 2006-07-18 | cardiac_m06 | | Controlling Chaos in the Heart. Shock Energy is Decreased >10 Times. What is next? | Yes | Yes |
| 2006-04-27 | joint98 | | Why We Should Believe in the Next-to-Minimal Supersymmetric Standard Model | Yes | No |
| 2006-03-06 | grb06 | | Cataclysmic and Catastrophic Cosmic Explosions: The Next Frontier[Podcast][Aud][Cam] KITP Blackboard Lunch | Yes | No |
| 2004-10-20 | colloq | | Planning Astronomy's Next Big Machines: Reflections on Some Recent History | Yes | Yes |
| 2004-01-14 | collider_c04 | | Next-to-Leading Order QCD Programs: Status and Prospects | No | Yes |
| 2002-11-08 | cmb02 | | After Acoustic Peaks: Next Generation CMB | No | No |
| 2001-11-13 | nano01 | | The Next Generation of Atomic-Force Microscopes | No | No |
| 1999-03-19 | gamma_c99 | | Next Generation GRB exp. approaches (20 min) | No | No |
| 1999-03-17 | gamma_c99 | | A jet-disk symbiosis model for GRB: Is SS433 next? | No | Yes |
| 1998-03-04 | colloq | | The Next Generation Cosmic Microwave Background Measurements and What We Hope to Learn About the Early Universe | No | Yes |