CMB B-mode - NEXT

27 janv. 2025, 09:30 → 29 janv. 2025, 18:00 Asia/Tokyo

Seminar Hall (KEK, Tsukuba - Building 3)

Guillaume Patanchon (ILANCE), Masaya Hasegawa (KEK-IPNS)

This workshop is organized as a collaboration between:

1. CMB-Inflate program - funded by European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No 101007633,
2. JSPS Core-to-core Program - Exploration of the origin and evolution of matter and space time: a research consortium for cosmic microwave background, PI Akito Kusaka,
3. The KEK Institute of Particle and Nuclear Studies KEK-IPNS,
4. The International Center for Quantum-field Measurement Systems for Studies of the Universe and Particles WPI-QUP.

The goals of this workshop are:

1. Review the latest results in CMB science
2. Define synergies between space-based and ground-based CMB measurements, data analysis, component separation and instrument development and modeling.
3. Following the core principles of the CMB-Inflate and Core-to-core programs, create strong international bonds between researchers and promote younger generations.

Zoom link for remote attendance: 

• https://us02web.zoom.us/j/87235264445?pwd=zr3hL6sKfHAllimokbcu5mJ6bRwOax.1
• Meeting ID: 872 3526 4445
• Passcode: 236700

 

KEKworkshop.pptx

lun. 27 janvier

09:30 → 09:45 Coffee

09:45 → 09:50 Logistics

Orateur: Tommaso Ghigna (QUP-KEK)

Welcome & Logistics

09:50 → 10:00 Opening Remarks

Orateur: Prof. Naohito Saito (KEK-IPNS)

10:00 → 10:25 CMB Polarization measurements with BICEP/Keck

Orateur: Kimmy Wu (SLAC National Accelerator Laboratory)

BICEP/Keck

10:25 → 10:50 Simons Observatory

Orateur: Junna Sugiyama (University of Tokyo)

Simons Observatory

10:50 → 11:10 Coffee Break

11:10 → 11:35 CMB-S4

Orateur: Clarence Chang (Argonne)

CMB-S4

11:35 → 12:00 LiteBIRD mission and its status

Orateur: Ryuichi Fujimoto (ISAS-JAXA)

LiteBIRD Status

12:00 → 13:30 Poster Session

13:30 → 14:30 IPNS Seminar: Observing the First Light in the Universe, from the Earth and from the Sky

Since Penzias and Wilson discovered the cosmic microwave background (CMB) in 1964, observation of CMB has been central to the development of modern and precision cosmology. Combined with other probes, it has told us so many things about the Universe - how the Universe began, how the Universe has evolved, what the universe is made of, and still, how many questions are unsolved about the Universe. Throughout its history, the CMB observation has gone through a unique progression - ground-based telescopes, balloon-borne telescopes, and space missions have helped one another and contributed to scientific advancement in their own ways. I am new to the field compared to the history, and I may be out of my depth, but I will make my attempt to review this history and the nature of the CMB observation to realize the synergy between the observations from the ground and the sky. This leads us to the discussion relevant today: how the CMB observations from the ground and the sky may work together now and in the future. I will review the synergies and complementarity between these different approaches, with a focus on CMB polarization measurements, and conclude with a promising outlook for the field.

Orateur: Akito Kusaka (University of Tokyo)

Akito's IPNS Seminar

14:30 → 15:00 Birefringence

Orateur: Ippei Obata (Kavli IPMU)

Birefringence

15:00 → 15:30 CMB detectors & readout and how to model them in data analysis

Orateur: Tijmen de Haan (KEK-IPNS & QUP)

Detector and Readout

15:30 → 16:00 Coffee Break

16:00 → 16:30 Synergy Between CMB and LSS

Orateur: Hironao Miyatake (Nagoya University)

CMB x LSS

16:30 → 17:00 Synergy Between Space and Ground Based Observations: Instruments

Orateur: Aritoki Suzuki (LBNL)

Synergy Instrument

17:00 → 17:30 Synergy Between Space and Ground Based Observations: Data Analysis

Orateur: Luca Pagano (Universita' di Ferrara)

Synergy Data

mar. 28 janvier

09:30 → 10:00 Coffee

10:00 → 11:00 Basics of TES microcalorimeter/bolometer and non-astronomy applications

Orateur: Kazuhisa Mitsuda (QUP)

TES Applications

11:00 → 11:20 Coffee Break

11:20 → 12:15 Machine Learning and Artificial Intelligence

12:15 → 13:30 Lunch

13:30 → 15:30 Galactic Foregrounds and Component Separation

15:30 → 16:00 Coffee Break

16:00 → 17:45 Instrument Modeling and Systemtic Effects

mer. 29 janvier

09:30 → 10:00 Coffee

10:00 → 10:30 Neutrino Physics

Orateur: Volodymyr Takhistov (QUP)

10:30 → 11:00 Instrument Modeling and Systemtic Effects

11:00 → 11:20 Coffee Break

11:20 → 12:20 Instrument Modeling and Systemtic Effects

12:20 → 13:30 Lunch

13:30 → 15:30 Data Analysis Techniques and Mitigation of Instrumental Effects

15:30 → 15:50 Coffee Break

15:50 → 17:20 Likehood and global analysis

17:20 → 17:35 Closing Remarks

Orateurs: Guillaume Patanchon (APC), Tommaso Ghigna (QUP-KEK)

Closing Remarks