Extended Source Diffraction Effects near Gravitational Lens Fold Caustics
Author(s) -
S. A. Zabel,
J. B. Peterson
Publication year - 2003
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 - 10.1086/376896
Subject(s) - diffraction , gravitational lens , physics , caustic (mathematics) , optics , brightness , astrophysics , fold (higher order function) , galaxy , redshift , computer science , mathematical physics , programming language
Calculations are presented detailing the gravitational lens diffraction dueto the steep brightness gradient of the limb of a stellar source. The lensingcase studied is the fold caustic crossing. The limb diffraction signal greatlyexceeds that due to the disk as a whole and should be detectable for whitedwarf sources in our Galaxy and it's satellites with existing telescopes.Detection of this diffraction signal would provide an additional mathematicalconstraint, reducing the degeneracy among models of the lensing geometry. Thediffraction pattern provides pico-arcsecond resolution of the limb profile.Comment: 19 pages including 17 figures, Accepted for publication in ApJ, Minor conceptual change from previous versio
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