Oct. 28, 2024
09:55 Welcome
10:00 Indira Ocampo : Neural Networks for cosmological model selection and feature importance using Cosmic Microwave Background data
10:30 Koichiro Nakashima : Revealing the “past” Dark Matter Density through Convolutional Neural Networks
11:00 George Alestas : Observational Constraints on Curvature-Assisted Quintessence and the α-Attractor Inflationary Models
11:30 Lunch (and Evacuation event)
13:30 Ryoto Inui : Gravitational lensing of gravitational waves
14:00 Yurino Mizuguchi : STOLAS: STOchasitc LAttice Simulation
14:30 Marienza Caldarola : Astrometric constraints on stochastic gravitational wave background with neural networks
15:00 coffee
15:30 Keitaro Ishikawa : Machine Learning for Emulating Halo Correlations
16:00 Savvas Nesseris : Machine learning tests of the cosmological constant model and beyond
16:30 Shogo Masaki : First confirmation of anisotropic bias from statistically anisotropic matter distributions
17:00 discussion and closing
Indira Ocampo (IFT)
Koichiro Nakashima (Nagoya)
George Alestas (IFT)
Ryoto Inui (Nagoya)
Keitaro Ishikawa (Nagoya)
Marienza Caldarola (IFT)
Yurino Mizuguchi (Nagoya)
Savvas Nesseris (IFT)
Kazuya Furusawa (Nagoya)
Kiyotomo Ichiki (Nagoya)
Atsushi J. Nishizawa (Gifu Shotoku/ Nagoya)
Nagoya University, Higashiyama Campus, ES606 (6th floor of the ES building, C2-4 in the campus map)
Kiyotomo Ichiki
Savvas Nesseris
Atsushi J. Nishizawa