Statistical Analysis of Random Fields in Cosmology
from
Monday, 4 March 2024 (01:20)
to
Wednesday, 6 March 2024 (17:40)
Monday, 4 March 2024
10:20
Registration
Registration
10:20 - 10:50
10:50
Opening
Opening
10:50 - 11:00
11:00
11:00 - 12:00
Contributions
11:00
Peak height distributions of Gaussian random fields and their statistical applications
-
Dan Cheng
12:00
Lunch
Lunch
12:00 - 13:20
13:20
13:20 - 14:40
Contributions
13:20
Minkowski functionals for isotropic random fields in the Euclidean space and the sphere
-
Satoshi Kuriki
14:00
Application of Minkowski functional to high energy physics and deep learning
-
Mihoko Nojiri
14:40
Tea time
Tea time
14:40 - 15:00
15:00
15:00 - 16:00
Contributions
15:00
Minkowski Tensors in Cosmology
-
Changbom Park
16:10
16:10 - 17:30
Contributions
16:10
Precision cosmology with big data
-
Masahiro Takada
16:50
Weak lensing analysis
-
Masamune Oguri
Tuesday, 5 March 2024
09:30
09:30 - 10:50
Contributions
09:30
Data analysis methods for the Cosmic Microwave Background (CMB) polarization
-
Yuji Chinone
10:10
Astronomy and Data Science
-
Shiro Ikeda
11:00
11:00 - 12:00
Contributions
11:00
Learning from Topology: Cosmological Parameter Inference from the Large-scale Structure
-
Gary Shiu
12:00
Photo
Photo
12:00 - 12:05
12:05
Lunch
Lunch
12:05 - 13:20
13:20
13:20 - 14:40
Contributions
13:20
Non-Gaussian Statistics for Non-Gaussian Fields
-
Jia Liu
14:00
Data Scientific Approach to the Large-Scale Structure in the Universe
-
Tsutomu Takeuchi
14:40
Tea time
Tea time
14:40 - 15:00
15:00
15:00 - 16:00
Contributions
15:00
Exploring the Potential of 3D Scene Reconstruction Techniques in Astronomy
-
Chiaki Hikage
16:10
16:10 - 17:30
Contributions
16:10
image based cosmology on the large-scale structure
-
Atsushi J. Nichizawa
16:50
21cm cosmology with machine learning
-
Hayato Shimabukuro
18:00
Banquet
Banquet
18:00 - 21:00
https://andryu.owst.jp/
Wednesday, 6 March 2024
09:30
09:30 - 10:50
Contributions
09:30
Consistency relations of the kurtosis in large scale structure and modified gravity
-
Sora Yamashita
10:10
Emulators for cosmological inference
-
Takahiro Nishimichi
11:00
11:00 - 12:00
Contributions
11:00
Interpretable reduced modeling of large-scale pattern dynamics - from materials science to astrophysics -
-
Yoh-ichi Mototake
12:00
Lunch
Lunch
12:00 - 13:20
13:20
13:20 - 14:40
Contributions
13:20
How much information is left in galaxy clustering beyond the power spectrum?
-
Kazuyuki Akitsu
14:00
Field-level inference with differentiable GridSPT
-
Ken Osato
14:40
Tea time
Tea time
14:40 - 15:00
15:00
15:00 - 16:20
Contributions
15:00
Galaxy shape/alignment statistics as a novel cosmological probe
-
Atsushi Taruya
15:40
Symmetry breaking in the large scale distribution of spin vector of galaxies?
-
Masanori Iye