xmmclusters

	Clusters in the XMM-COSMOS field

News and Updates

May 11th, 2004: The latest results for the Subaru selected cluster are (assuming a spectroscopic redshift of 0.73 provided by the Bologna group):

Gas mass	err	kT	errs	density	err	entropy	err	pressure	err	inner radius (Mpc)	outer radius (Mpc)
1.177E+13	7.934E+11	2.929	-0.6 +0.9	1.108E-03	7.467E-05	273.5	75.7	5.200E-12	1.463E-12	0.000	0.466

May 10th, 2004: In a recent email, Alexis Finoguenov has pointed out the methods to apply to the XMM data for the cluster finding project and an estimate of the time scale to get results. A copy of the above mentioned email can be found here.

April 28th, 2004: First results of the galaxy-to-XMM comparison by Alexis Finoguenov and Nick Scoville can be found here:

April 15th, 2004: XMM contours on the Subaru selected cluster at z~0.6.

April 15th, 2004: XMM detection of a group/cluster at z~0.15 superimposed on a Subaru R image (Fig 1). An analysis of the group was carried out by Alexis Finoguenov (see Fig 2)


Fig 1	Fig 2

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Page manteined by I. Matute. Last updated on May 11th, 2004