Program

June 10 (Mon)
10:00-10:15 Opening Talk (Chair: Hideyuki Tagoshi)

       Takaaki Kajita (ICRR)

10:15-11:50 Plenary Talk (Chair: Hideyuki Tagoshi)


       Hyung Mok Lee (SNU), "KGWG Activities"

       Kazuaki Kuroda (ICRR), "Overview on Current Status of KAGRA"


11:50-13:00 Lunch


13:00-15:05 Instrument (Chair: Nobuyuki Kanda)


       Norikatsu Mio (UTokyo), "Laser"

	Shinji Miyoki (ICRR), "Interferometer"

	Kyuman Cho (Sogang Univ.), "Precision tilt sensor using double-pass AOM

       Ryutaro Takahashi (ICRR, NAOJ), "Vibration isolation"

	Sang-Pyo Kim (Kunsan National Univ.), "Gravitational Wave-Matter
Interactions and Quantum Mesurement"

15:05-15:35 Coffee Break

15:35-18:05 Data Analysis (Chair: Hyung Won Lee)

	Hideyuki Tagoshi (Osaka Univ.)

	Nobuyuki Kanda (Osaka City Univ.)

	Yousuke Itoh (UTokyo)

	Heesuk Cho (Pusan National Univ.), "Effective Fisher Matrix:
Semi-analytic Approach to the Parameter Estimation Accuracy"

	Chunglee Kim (SNU), "Markov-Chain Monte Carlo parameter estimation of
CBC inspirals"

	Kyungmin Kim (Hanyang Univ./ NIMS), "CBC GRB MVC"


18:30-20:30 Banquet


June 11 (Tue)

10:00-10:50 Theory (Chair: Kazuhiro Hayama)

	Hyung Won Lee (Inje Univ.), "Stochastic gravitational wave and its
spectral property"

	Changhwan Lee (Pusan National Univ.), "Neutron Star Mass Distribution
in Binaries"

10:50-11:50 Detector Characterization (Chair: Kyuman Cho)

	Kazuhiro Hayama (Osaka City Univ.)

	Young-Min Kim, Sang-Hoon Oh, John J. Oh, and Edwin J. Kim  (NIMS),
"Noise Identification in gravitational wave search using Artificial
Neural Networks"


11:50-13:00 Lunch

13:00-13:50 Discussion about the future collaboration (Chairs: Seiji
Kawamura and Hyung Mok Lee)

13:50-14:00 Closing Talk

       Hyung Mok Lee (SNU)



==============================================================

 Meeting Jun 10 13:00-15:00 

[John Oh]
To add my short comments, we are going to compare trigger generation performance by HHT to KW triggers using CLIO data.

[SangHoon Oh]
Since, Edwin and John have been testing HHT (Hilbert Huang Transform) on a few aux channels in RDS data set, we might able to generate HHT triggers from the hoft data from CLIO and compare those with KW triggers. If you can provide any single PEM channel, that would be better. There still remains a long way to go before we can generate HHT triggers, Let's give it a try. :-)