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Strong Lensing Reconstruction
- Source :
- The Astrophysical Journal. 534:L19-L22
- Publication Year :
- 2000
- Publisher :
- American Astronomical Society, 2000.
-
Abstract
- We present a general linear algorithm for measuring the surface mass density 1-\kappa from the observable reduced shear g=\gamma/(1-\kappa) in the strong lensing regime. We show that in general, the observed polarization field can be decomposed into ``electric'' and ``magnetic'' components, which have independent and redundant solutions, but perfectly orthogonal noise properties. By combining these solutions, one can increase the signal-to-noise ratio by \sqrt{2}. The solutions allow dynamic optimization of signal and noise, both in real and Fourier space (using arbitrary smoothing windows). Boundary conditions have no effect on the reconstructions, apart from its effect on the signal-to-noise. Many existing reconstruction techniques are recovered as special cases of this framework. The magnetic solution has the added benefit of yielding the global and local parity of the reconstruction in a single step.<br />Comment: final accepted version for ApJL
- Subjects :
- Physics
Astrophysics (astro-ph)
Mathematical analysis
FOS: Physical sciences
Astronomy and Astrophysics
Observable
Single step
Astrophysics
Polarization (waves)
01 natural sciences
Linear algorithm
Space and Planetary Science
Frequency domain
0103 physical sciences
Boundary value problem
010306 general physics
010303 astronomy & astrophysics
Surface mass
Smoothing
Subjects
Details
- ISSN :
- 0004637X
- Volume :
- 534
- Database :
- OpenAIRE
- Journal :
- The Astrophysical Journal
- Accession number :
- edsair.doi.dedup.....1376adaefaf412ffa4b418b470319ec4