Monday August 11th |
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Opening Session (08:30 - 09:00) |
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Conference photograph |
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09:15 - 09:45 Coffee Break |
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Session #1: Large Scale Structures (09:45 - 11:45) |
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The Dark Energy Spectroscopic Instrument: Cosmological results from the Data Release 2
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DESI and the Neutrino Frontier
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LSST: From First Light to Mapping the Cosmos
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12:00 - 13:30 Lunch |
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Session #2: Cosmic Microwave Background (13:30 - 14:45) |
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Astrophysics and cosmology with the South Pole Telescope: recent results and future directions
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The Subaru Prime Focus Spectrograph Cosmology Program
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14:45 - 15:15 Coffee Break |
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15:15 - 16:30 Panel discussion on Large Surveys |
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16:30 - 18:00 Informal discussions and/or beach |
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Tuesday August 12th |
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Session #4: Theory (08:30 - 10:00) |
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Searching for Inflationary Physics with the CMB Trispectrum
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Dark dimension cosmology
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RockStar Baryogenesis: Baryogenesis from primordial CP violation
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10:00 - 10:30 Coffee Break |
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Session #5: Cosmic Microwave Background (10:30 - 12:00) |
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Cosmic Birefringence and Its Implications for Physics beyond the Standard Model
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Dust polarization results from Planck
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Constraints on primordial non-Gaussianity from CMB lensing cross-correlations with DESI and Quaia data
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12:00 - 13:30 Lunch |
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Session #6: Other Probes (13:30 - 15:00) |
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The nHz Gravitational Wave Background: Evidence and Open Questions
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Cosmology with Line Intensity Mapping from Antartica with SPT-SLIM and TIM
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Fundamental Physics and Cosmology with TianQin
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15:00 - 15:30 Coffee Break |
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Session #7: Other Probes (15:30 - 16:50) |
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Constraining primordial black holes using gravitational wave observations
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Tuning the cosmic instrument: robust cosmology through combined probes
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YOLO-CL : Deep Machine Learning for Galaxy Cluster detection with LSST
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16:50 - 18:00 Informal discussions and/or beach |
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Wednesday August 13th |
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Session #8: Large Scale Structures (08:30 - 10:00) |
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Dark Energy Survey: implications for cosmological expansion models from the final DES Baryon Acoustic Oscillation and Supernova data
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Cosmology from weak lensing and galaxy clustering in the Dark Energy Survey
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KiDS-Legacy: Cosmic shear results from the complete Kilo-Degree Survey
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10:00 - 10:30 Coffee Break |
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Session #9: Large Scale Structures (10:30 - 11:40) |
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Time-domain Cosmology in the Era of Large Surveys
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Inference of Weak Lensing Parameters from Blended Galaxies Using Generative Neural Networks
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Cosmology with Quasar Proper Motions: Constraining Anisotropic Expansion of the Universe
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12:00 - 13:30 Lunch |
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14:00 - 18:30 Excursions For Ky Co excursion, please give the ICISE staff the informations requested in this file |
Thursday August 14th |
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Session #10: Large Scale Structures (08:30 - 10:00) |
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Simulation-Based Inference for Cosmology
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The challenges of using Baryon Acoustic Oscillations distances for cosmology
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Positive neutrino masses with DESI DR2 via matter conversion to dark energy
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10:00 - 10:30 Coffee Break |
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Session #11: Hidden Sector (10:30 - 11:50) |
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Populating Hidden Sectors through Gravitational Particle Production
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(Runaway) Gravitational Production of Dark Photons
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Generalized bulk-flow on computing gravitational wave background from first order phase transition
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12:00 - 13:30 Lunch |
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Session #12: Dark Matter Models (13:30 - 15:00) |
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Secondary gravitational waves and the early universe
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Galaxy evolution, observational biases and cosmological tensions
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Probing Particle Physics with the Cosmological Collider
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15:00 - 15:30 Coffee Break |
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Session #13: H0 Tensions (15:30 - 16:30) |
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The Hubble parameter of the Local Distance Ladder from dynamical dark energy with no free parameters
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A New Master Supernovae Ia sample and the investigation of the H0 tension
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16:30 - 17:30 Panel discussion |
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18:30 - 21:00 Conference Dinner at ICISE |
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Friday August 15th |
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Session #14: Cosmic Microwave Background (08:30 - 09:50) |
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Untangling dust and CIB emission in Planck 353 GHz observation with Scattering Coefficients
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Simons Observatory
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CMB-Bharat: A perspective for an Indian role in Cosmic enterprise
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09:50 - 10:10 Coffee Break |
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Session #15: Cosmic Microwave Background (10:10 - 11:30) |
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The LiteBIRD mission: probing inflation with CMB polarization
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Large-Scale Polarization Measurements of the Cosmic Microwave Background: From Planck to LiteBIRD
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Semi-blind component separation for measurement of CMB B-mode polarization
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11:30 - 12:30 Visit of Explora Science |
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12:30 - 14:00 Lunch |
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Closing Session (14:00 - 15:00) |
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Outlook/Perspectives/Vision
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15:00 - 15:30 Coffee Break |
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15:30 - 17:00 Fruit Party on the beach |
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18:30 Dinner at ICISE |
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Last modification 15/08/25 (jdz)