- The maximum size of the poster is A0. The direction must be vertically long (i.e., upright format)
- Victor Chan (Univ. of Toronto), “Simulating the effects of detector crosstalk on future CMB observations”
- Fabio Columbro (Sapienza Univ. di Roma), “LiteBIRD-MHFT polarization modulator units: progress update”
- Josquin Errard (APC/CNRS, France), “A framework for performance forecasting of the parametric component separation in the presence of achromatic HWP and sinuous antennas effects”
- Hiroaki Imada (LAL/CNRS, France), “Beam pattern simulation including a wave plate”
- Greg Jaehnig (Univ. of Colorado Boulder, USA), “Design and Characterization of Transition-Edge Sensor Bolometers for LiteBIRD”
- Kunimoto Komatsu (Okayama Univ., Japan), “Demonstration of mm-wave performance of small prototype LiteBIRD LFT AHWP at around 20K”
- Tomotake Matsumura (Kavli IPMU, Japan), “Current status of the inflight beam calibration study and the future plan”
- Yoshiki Nomura (Saitama Univ., Japan), “Characterization of the energy loss of a ferromagnetic material for LiteBIRD polarization modulator”
- Hiroki Ochi (Yokohama National Univ., Japan), “Estimating the Upper Limit on CMB Circular Polarization from LiteBIRD”
- Shinya Sugiyama (Saitama Univ., Japan), “Development of the prototype onboard FPGA to reconstruct the position angle of the LiteBIRD PMU HWP using optical encoder”
- Ryota Takaku (Univ. of Tokyo, Japan), “The development of SWS as a broadband AR in a large area using laser ablation for LFT HWP”
- Hayato Takakura (Univ. of Tokyo, ISAS/JAXA, Japan), “Far-sidelobe and Polarization Measurements of LiteBIRD Low Frequency Telescope Scaled Model”
- Patricio Vielva (Instituto de Física de Cantabria (CSIC-UC), Spain), “A calibration satellite for ultra-sensitivity CMB polarization space missions”
- Patricio Vielva (Instituto de Física de Cantabria (CSIC-UC), Spain), “On the Detection of Primordial CMB B-modes from Ground at Low Frequency”
- Patricio Vielva (Instituto de Física de Cantabria (CSIC-UC), Spain), “On the Delensing of the Cosmic Microwave Background Polarization”