Subjects (H24-H25)
Group | Affiliation | Leader | Title |
---|---|---|---|
A01 | Tsukuba University | Suguru Takada | Development of bobbin-less superconducting magnet and multilayer magnetic shields for high efficient ADR |
A01 | NIMS | Takenori Numazawa | Multi-stages ADR system for space missions |
A01 | KEK | Masaya Hasegawa | Laboratory Calibration System for Large Focal Planes with Superconducting CMB Detectors |
A01 | KEK | Tomotake Matsumura | Development of a continuously rotating broadband half-wave plate modulator for a cosmic microwave background polarization experiment |
A02 | NAOJ | Takeshi Noguchi | Development of a low-noise microwave kinetic inductance detector(MKID) |
A02 | NAOJ | Ken'ichi Karatsu | Construction of beam measurement system for integration of MKID camera array |
A02 | KEK | Mitsuhiro Yoshida | |
A03 | The University of Tokyo | Kimiaki Kawara | Observations of the Cosmic Optical Background |
A03 | JAXA | Kouji Tsumura | Absolute Measurement of the Cosmic Near-Infrared |
A04 | Chiba University | Ryouji Matsumoto | Background Using Eclipsed Galilean Satellites as Occulters |
A04 | Nagoya University | Tsutomu Takeuchi | A study on the CMB foreground decomposition by the self-organizing state-space model |
A05 | Tohoku University | Fuminobu Takahashi | Non-Gaussianity as a probe of the origin and evolution of density perturbation |
A05 | Tokyo Institute of Technology | Masahide Yamaguchi | Constraints on inflation models from non-Gaussianities of primordial density and tensor fluctuations |
A05 | Kyoto University | Takahiro Tanaka | Quantum fields on inflationary spacetime |
A05 | Kumamoto University | Keitaro Takahashi | Probing Early Universe with Cosmic Strings |
Subjects (H22-H23)
Group | Affiliation | Leader | Title |
---|---|---|---|
A01 | Kinki University | Izumi Ohta | Development of the wide-viewing broadband optical system for the polarization observation of the cosmic background radiation |
A01 | KEK | Nobuhiro Kimura | Development of a ultra lightweight High Tc superconducting magnet for space-flight ADR |
A01 | KEK | Nobu Katayama | Development of analysis pipeline using Fermi GPUs |
A01 | KEK | Mitsuhiro Yoshida | Sub-diffraction-limit millimeter wave optics for sattelite using micro-structure including super lens |
A01 | KEK | Masaya Hasegawa | Study of polarized foreground emission for the future satellite CMB experiment |
A01 | JAXA | Yoh Takei | Innovational multiplexing readout of transition edge sensors for study of structure formation and evolution of the Universe |
A02 | Nagoya University | Hiroyuki Akaike | Development of high quality NbN junctions with plasma-nitrided barriers for submillimeter-wave detectors with high sensitivity |
A03 | The University of Tokyo | Kimiaki Kawara | Obseravtions of the Cosmic Optical Background |
A03 | Kyoto University | Tomonori Totani | Developing Cosmological Galaxy Formation Model in Infrared Regime |
A05 | Hirosaki University | Ryuichi Takahashi | Estimating E-mode polarization induced by gravitational lensing using ray shooting simulations |
A05 | Yamagata University | Nobuyuki Sakai | Imprints of Nonlinear Large Scale Structure on Cosmic Microwave Background Radiation and Their Constraints on Early-Universe Models |
A05 | The University of Tokyo | Fuminobu Takahashi | Cosmology in the low-scale inflation and its observational implications |
A05 | Kyoto University | Takahiro Tanaka | Infrared and Ultraviolet divergence problem in inflation |