SUMMARY OF PROPOSAL 41271
DR TAKESHI GO TSURU
KYOTO UNIV.
KYOTO JAPAN 606-01
KYOTO
KITASHIRAKAWA

  E-mail: TSURU@CR.SCPHYS.KYOTO-U.AC.JP	Tel: (81)-75-753-3843	Fax: (81)-75-701-5377
  Medium: 2.5GB8MM

Subject: CLUSTERS OF GALAXIES AND SUPERCLUSTERS                      
  Title: THE HIGH RESOLUTION MULTI-WAVELENGTH SURVEY PROGRAM OF THE DISTANT MASSIVE ROSAT ALL-SKY-SURVEY CLUSTERS


Abstract:
 Clusters of galaxies are key objects for understanding the origin and growth of
 structure in the universe. Measurement of temperature of ICM with ASCA are ideal for
 studying the potential wells, and thus the dynamical state, of these massive
 systems. We have selected 8 objects from the ROSAT All Sky Survey and undertaken to
 obtain a complete set of high resolution follow-up observations including studies of
 X-ray morphology, optical spectroscopy/photometry, and radio and IR measurements of
 cluster galaxies, which provides deep insights into the structures and coherent
 picture of young cluster environments. All observations except for ASCA have already
 finished. The porject will be complete by the observations of ASCA.

 Co-Is:
   1  M. PIERRE           	SACLAY                        FRANCE    
      (No Co-I contact data)
   2  J. HUGHES           	CFA                           USA       
   3  R. HUNSTEAD         	SYDNEY                        AUSTRALIA 
   4  Y. MELLIER          	TOULOUSE                      FRANCE    
   5  K. KOYAMA           	KYOTO                         JAPAN     
   6  H. EBELING          	CAMBRIDGE                     UK        


Target Name           PRI RA        Dec        Time TC  Off GIS SIS_Cts  Obs
-------------------   --- --------  --------   ---- --  --- --- -------  ---
PRG32 (A1111)          1  162.6458   -2.6042    30   N   Y   P  0.33000   1 

REMARKS:  IF ALL THE EXPOSURE WE APPLY IS NOT ACCEPTABLE, PLEASE DO NOT REDUCE NO.
          OF TARGETS BUT REDUCE EXPOSURE OF EACH TARGET AND KEEP NO. OF TARGETS.
PRG74                  1  198.6333  -25.2672    70   N   Y   P  0.11000   1 

REMARKS:  IF ALL THE EXPOSURE WE APPLY IS NOT ACCEPTABLE, PLEASE DO NOT REDUCE NO.
          OF TARGETS BUT REDUCE EXPOSURE OF EACH TARGET AND KEEP NO. OF TARGETS.