|
Size: 2025
Comment:
|
Size: 2100
Comment:
|
| Deletions are marked like this. | Additions are marked like this. |
| Line 15: | Line 15: |
| ||11:00-11:30 ||Verification of cooling time reduction for KAGRA ||SAKAKIBARA, Yusuke || || | ||11:00-11:30 ||Verification of cooling time reduction for KAGRA ||SAKAKIBARA, Yusuke ||[[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/DocDB/ShowDocument?docid=1637|O]] || |
Opening a new era for the astrophysics: The future detectors of gravitational waves
Date: Apr 19(Fri), 2013
Location and access: Italian Institute of Culture, Tokyo
More information on the meeting is here.
Program
Apr 19 (Fri.) |
|||
|
|
||
Time |
Title |
Speaker |
File |
|
|
|
|
10:00-10:05 |
Welcome |
CRISAFULLI, Edoardo |
|
10:05-10:10 |
Welcome |
MENGONI, Alberto |
|
10:10-10:30 |
From Virgo to ET |
PUNTURO, Michele |
|
10:30-11:00 |
Introduction of the recent progress in Japan |
YAMAMOTO, Kazuhiro |
|
11:00-11:30 |
Verification of cooling time reduction for KAGRA |
SAKAKIBARA, Yusuke |
|
11:30-12:00 |
Low Noise Optical Coatings for Advanced GW Detectors |
PINTO, Innocenzo M |
|
12:00-12:30 |
Coatings in Advanced Virgo and beyond |
FLAMINIO, Raffaele |
|
12:30-13:00 |
Alignment Sensing and Control for KAGRA |
MICHIMURA, Yuta |
|
|
|
|
|
Lunch time 13:00~14:30 |
|||
|
|
|
|
14:30-14:50 |
Coating research in ELiTES |
CRAIG, Kieran |
|
14:50-15:20 |
Suspensions in Advanced Virgo and comparison with KAGRA |
MAJORANA, Ettore |
|
15:20-15:50 |
Development Status of Seismic Attenuation System for KAGRA |
SEKIGUCHI, Takanori |
|
15:50-16:20 |
Vibration measurement of the KAGRA radiation shield |
CHEN, Dan |
|
16:20-16:50 |
Torsion-bar Antenna and Its Collaboration with Interferometers |
SHODA, Ayaka |
|
16:50-17:10 |
Mechanical Loss and Thermal Conductivity of Materials for KAGRA and ET |
HOFMANN, Gerd |
|
17:10-17:30 |
Conclusive Remarks |
KAJITA, Takaaki |
|
|
|
|
|