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Looking at the Fundamental Plane through a Gravitational Lens
Author(s) -
G. Bertin,
Marco Lombardi
Publication year - 2006
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/507298
Subject(s) - physics , gravitational lens , mass distribution , fundamental plane (elliptical galaxies) , galaxy , lens (geology) , gravitation , plane (geometry) , dimensionless quantity , degeneracy (biology) , galaxy cluster , measure (data warehouse) , astrophysics , elliptical galaxy , classical mechanics , optics , geometry , lenticular galaxy , redshift , computer science , quantum mechanics , mathematics , biology , database , bioinformatics
We consider the Fundamental Plane of elliptical galaxies lensed by thegravitational field of a massive deflector (typically, a cluster of galaxies).We show that the Fundamental Plane relation provides a straightforwardmeasurement of the projected mass distribution of the lens with a typicalaccuracy of ~0.15 in the dimensionless column density kappa. The proposedtechnique breaks the mass-sheet degeneracy completely and is thus expected toserve as an important complement to other lensing-based analyses. Moreover, itsability to measure directly the mass distribution on the small pencil beamsthat characterize the size of background galaxies may lead to crucial tests forcurrent scenarios of structure formation.Comment: ApJL, in pres

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