Structure Formation and Cosmology with high-z Clusters
Lecture4 - USP
Lecture4 - USP
- No tags were found...
You also want an ePaper? Increase the reach of your titles
YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.
Can we extend this work beyond redshift one ?[...continues from Lecture 3]– Can we measure the DM distribution inz>1 clusters <strong>with</strong> sufficient accuracy ?!evolution of DM distribution– Can we then measure M200 of mostdistant clusters <strong>with</strong> sufficientaccuracy ?!mass calibration of future surveys!test !CDM <strong>with</strong> most massiveclusters N(>10 15 M!,z>1)