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Office of News and Information
Johns Hopkins University
901 South Bond Street, Suite 540
Baltimore, Maryland 21231
Phone: 443-287-9960 | Fax: 443-287-9920

December 9, 2005
FOR IMMEDIATE RELEASE
CONTACT: Lisa De Nike
(443) 287-9960
lde@jhu.edu


JHU-STScI Team Maps Dark Matter in
Startling Detail

Graphics

Dark matter in the high-redshift cluster CL 0152-1357. Gravitational lensing analysis with the Advanced Camera for Surveys (ACS) reveals the complicated dark matter distribution (purple) in unprecedented detail when the Universe was at half its present age. The yellowish galaxies are the visible cluster member galaxies forming a filamentary structure, possibly in the process of merging.
(Jee et al. 2005, Astrophysical Journal)

 

On the left hand side is an ACS image that shows the lensed galaxy elongated vertically by gravity. However, when the same galaxy is observed with the Very Large Telescope (VLT) at Cerro Paranal, we only see a small blob indicating no hints of lensing (right panel). The shape information has been destroyed by the atmospheric turbulence even if it is much weakerthere than at the sea level.

 

Holland Ford, Myungkook James Jee and Richard White

Go to News Release: JHU-STScI Team Maps Dark Matter in Startling Detail


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