September 7-9, 2019 Beijing, China
We are entering new era of the Cosmic Microwave Background research, aiming to probe the Primordial Gravitational Waves (PGWs) originated from the very early Universe. Recently, China has launched the Ali CMB Polarization Telescope (AliCPT) in Tibetan Plateau to measure CMB B-mode polarization in northern hemisphere. This symposium brings together experimental and theoretical scientists that are interested in contributing to this project. The program consists of plenary sessions with presentations covering, but not being limited to, the following topics:
* Foreground removal & novel techniques in CMB signal extraction;
* Simulation & computational development for the forthcoming data sets;
* Early universe theories & cosmological implications;
* Systematic effects & survey strategy;
* System hardware design & software design.
The aim of this symposium is to foster discussions and to exchange ideas among active researchers in this field.
If you have any questions, such as Visa, invitation letter etc., please contact:
Bin Hu (alicpt2019@gmail.com)
There is no registration fee, but advanced registration for the symposium is required. Thanks to support from the NSFC.
For non-ihep user, when you created account, please fill in the following contact person (Dr. Hong LI) email: hongli@ihep.ac.cn
Formal Registration and Abstract Submission
Registration deadline: August 16, 2019
Abstract submission deadline: August 23, 2019
Only registered participants can submit abstracts. It is recommended that participants register early in order for LOC to provide timely assistance (e.g. invitation letter for visa and hotel reservation) if needed.
Talks
Benjamin D. Wandelt Bin Hu Bin Yue Congzhan Liu Hao Liu Hong Li Jacques Delabrouille Jan Hamann Ji Yao Le Zhang Pawel Bielewicz Shamik Ghosh Shaul Hanany Wen Zhao Xian Gao Xiaodong Li Ye Cao Yu Gao Zhiqi Huang
Analysis techniques for CMB B-mode experiments CMB Lensing The cosmic infrared background (CIB) Current Status of AliCPT-1 Experiment EB-leakage and minimum variance estimation of the fullsky signal & spectrum Ali CMB Polarization Telescope Future Cosmic Mircrowave observations from Space: A European perspective CMB Lensing and Minkowski Functionals The power of CMB-lensing: AliCPT x DESI & more ... Foreground removal pipeline in AliCPT Testing significance of the large angular scale CMB anomalies The hemispherical power asymmetry after Planck PICO Translating observed (Q,U)-maps to B-mode power spectrum and scientific results: Constructing the optimal estimators Propagation of gravitational waves in a cosmological background Cosmic large-scale structure deep learning Auto- and cross-correlation of the cosmic microwave background lensing and infrared background measured by Planck and Hershel Testing dark matter energy injection in CMB measurements Primordial fluctuations and rare objects in the universe
BNU Campus Map
INVITED SPEAKER
Confirmed
Jacques Delabrouille (CNRS)
Martin Bucher (CNRS)
Jan Hamann (UNSW)
Shaul Hanany (U Minnesota)
Fabio Finelli (INAF BOLOGNA)
Pawel Bielewicz (NCNR)
Chang Feng (UIUC)
SCIENTIFIC ORGANIZING
COMMITTEE
Xinmin Zhang (IHEP)
Jacques Delabrouille (CNRS)
Jian-Ping Cheng (BNU)
Chao-Lin Kuo (Stanford)
Albert Stebbins (Fermilab)
Gary Shiu (UW-Madison)
Gregory Tucker (Brown)
Peter Timbie (UW-Madison)
Benjamin D. Wandelt (Flatiron)
LOCAL ORGANIZING
COMMITTEE
Bin Hu (BNU)
Hong Li (IHEP)
Ki Won Yoon (Stanford)
Jun-Qing Xia (BNU)
Bin Yue (NAOC)
Le Zhang (SJTU)
Yi-Fu Cai (USTC)
Jia-Yong Zhong (BNU)
